References from Interstellar Turbulence I: Observations and Processes
Authors: Bruce Elmegreen & John Scalo
Adler DS, Roberts WW Jr. 1992. Ambiguities in the identification of giant molecular
cloud complexes from longitude-velocity diagrams. ApJ. 384:95-104
Andreopoulos Y, Agui JH, Briassulis G. 2000. Shock wave-turbulence interactions.
Ann.Rev.Fluid Mech. 32:309-345
Anselmet F, Gagne Y, Jopfinger EJ, Antonia RA 1984. High order velocity structure
functions in turbulent shear flows. J. Fluid Mech. 140:63-89
Arons J, Max CE. 1975. Hydromagnetic Waves in Molecular Clouds. ApJ. 196:L77L81
Avila-Reese V, Vazquez-Semadeni E. 2001. Turbulent Dissipation in the Interstellar
Medium: The Coexistence of Forced and Decaying Regimes and Implications for Galaxy
Formation and Evolution. ApJ. 553:645-660
Ayyer A, Verma M. K. 2003. Energy transfer and locality in magnetohydrodynamic
turbulence. ArXiv: nlin.CD/0308005
Baker PL. 1973. A Statistical Investigation of Neutral Hydrogen Line Profiles. A&A.
23:81-92
Balbus SA, Hawley JF. 1991. A powerful local shear instability in weakly magnetized
disks. I - Linear analysis. II - Nonlinear evolution. ApJ . 376:214-222
Ballesteros-Paredes J. 2003. Turbulent Fragmentation and Star Formation Authors: Javier
Ballesteros-Paredes. astroph/0311319
Ballesteros-Paredes J, Vazquez-Semadeni E, Scalo J. 1999. Clouds as Turbulent Density
Fluctuations: Implications for Pressure Confinement and Spectral Line Data
Interpretation. ApJ. 515:286-303
Ballesteros-Paredes J, Hartmann L, Vazquez-Semadeni E. 1999. Turbulent Flow-driven
Molecular Cloud Formation: A Solution to the Post-T Tauri Problem? ApJ. 527:285297
Ballesteros-Paredes J, Mac Low M-M. 2002. Physical versus Observational Properties of
Clouds in Turbulent Molecular Cloud Models. ApJ. 570:734-748
Ballesteros-Paredes J, Vazquez-Semadeni E, Goodman, AA. 2002. Velocity Structure of
the Interstellar Medium as Seen by the Spectral Correlation Function. ApJ. 571:334355
Ballesteros-Paredes J, Klessen RS, Vazquez-Semadeni E. 2003. Dynamic Cores in
Hydrostatic Disguise. ApJ. 592:188-202
Bally J, Langer WD, Stark AA, Wilson RW 1987. Filamentary structure in the Orion
molecular cloud. ApJ. 312:L45-L49
Balsara D, Benjamin RA, Cox DP. 2001. The Evolution of Adiabatic Supernova
Remnants in a Turbulent, Magnetized Medium. ApJ. 563:800-805
Balsara DS, Crutcher RM, Pouquet A. 2001. Turbulent Flows within Self-gravitating
Magnetized Molecular Clouds. ApJ. 557:451-463
Balsara D, Ward-Thompson D, Crutcher RM. 2001. A turbulent MHD model for
molecular clouds and a new method of accretion on to star-forming cores. MNRAS.
327:715-720
Bania TM, Lyon JG. 1980. OB stars and the structure of the interstellar medium - Cloud
formation and effects of different equations of state. ApJ. 239:173-192
Barrat A, Trizac E. 2002. Molecular dynamics simulations of vibrated granular gases.
Phys. Rev. E. 66:051303-1-051303-13
Basu S, Murali C. 2001. Constraints on Stirring and Dissipation of MHD Turbulence in
Molecular Clouds. ApJ. 551:743-746
Bataille F, Zhou Y. 1999. Nature of the energy transfer process in compressible
turbulence. Phys. Rev. E. 59:5417-5426
Bate MR, Burkert A. 1997. Resolution requirements for smoothed particle
hydrodynamics calculations with self-gravity. MNRAS . 288:1060-1072
Bate MR, Bonnell IA, Bromm V. 2002. The formation of close binary systems by
dynamical interactions and orbital decay. MNRAS. 336:705-713
Bate MR, Bonnell IA, Bromm V. 2003. The formation of a star cluster: predicting the
properties of stars and brown dwarfs. MNRAS. 339:577-599
Bazell D, Desert FX. 1988. Fractal structure of interstellar cirrus. ApJ. 333:353-358
Beech M. 1987. Are LYNDS dark clouds fractals? Ap&SS. 133:193-195
Ben-Naim E, Krapivsky PL. 2002. Scaling, multiscaling, and nontrivial exponents in
inelastic collision processes. Phys. Rev. E. 66:011309-1-011309-10
Bensch F, Stutzki J, Ossenkopf, V. 2001. Quantification of molecular cloud structure
using the Delta -variance. A&A. 366:636-650
Beran MJ. 1968. Statistical continuum theories. New York: Interscience Publishers. 424
pp.
Berkhuijsen EM. 1999. Volume Filling Factors of ISM Phases and Turbulent Structure.
In Plasma Turbulence and Energetic Particles in Astrophysics. ed. M Ostrowski, R
Schlickeiser, pp. 61-65. Krakow: Obs. Astron. Uniw. Jagiellonski
Bertin G, Lodato G. 2001. Thermal stability of self-gravitating, optically thin accretion
disks. A&A . 370:342-350
Bertoglio JP, Bataille F, Marion JD 2001. Two-point closures for weakly compressible
turbulence. Phys. Fluids. 13:290-310
Bertoldi F, McKee CF. 1992. Pressure-confined clumps in magnetized molecular clouds.
ApJ. 395:140-157
Bhattacharjee A, Ng CS. 2001. Random Scattering and Anisotropic Turbulence of Shear
Alfven wave Packets. ApJ. 548:318-322
Biferale L. 2003. Shell models of energy cascade in turbulence. Ann. Rev. Fluid Mech.
35:441-468
Biferale L, Lanotte A, Toschi F. 2003. Effects of forcing in three dimensional turbulent
flows. nlin.CD/0310022
Biskamp D 2003. Magnetohydrodynamic turbulence. Cambridge: Cambridge Univ.
Press. 310 pp.
Biskamp D, Muller W-C. 1999. Decay Laws for Three-Dimensional
Magnetohydrodynamic Turbulence. Phys.Rev.Lett. 83:2195-2198
Biskamp D, Muller W-C. 2000. Scaling properties of three-dimensional isotropic
magnetohydrodynamic turbulence. Physics of Plasmas. 7:4889-4900
Biskamp D, Schwarz E. 2001. On two-dimensional magnetohydrodynamic turbulence.
Phys. Plasmas 8:3282-3292
Black DC, Matthews MS. Eds. 1985 Protostars and Planets II. Tucson: Univ. Ariz. Press
Blondin JM, Marks BS. 1996. Evolution of cold shock-bounded slabs. NewA . 1:235244
Bok BJ, Reilly EF. 1947. Small Dark Nebulae. ApJ. 105:255-257
Boldyrev, S. 2002. Kolmogorov-Burgers Model for Star-forming Turbulence. ApJ.
569:841-845
Boldyrev S. Nordlund A. Padoan P. 2002. Scaling Relations of Supersonic Turbulence in
Star-forming Molecular Clouds ApJ. 573:678-684
Boldyrev S, Nordlund A, Padoan, P. 2002. Supersonic Turbulence and Structure of
Interstellar Molecular Clouds. Phys. Rev. Lett. 89:031102-031102-4
Bonazzola S, Heyvaerts J, Falgarone E, Perault M, Puget JL. 1987. Jeans collapse in a
turbulent medium. A&A. 172:293-298
Bonazzola S, Perault M, Puget JL, Heyvaerts J, Falgarone E, Panis, JF. 1992. Jeans
collapse of turbulent gas clouds - Tentative theory. J. Fluid Mech. 245:1-28
Bonnell IA, Bate MR, Clarke CJ, Pringle JE. 1997. Accretion and the stellar mass
spectrum in small clusters. MNRAS. 285:201-208
Bonnell IA, Bate MR, Vine SG. 2003. The hierarchical formation of a stellar cluster.
MNRAS. 343:413-418
Bourke TL, Myers PC, Robinson G, Hyland AR. 2001. New OH Zeeman measurements
of magnetic field strengths in molecular clouds. ApJ. 554:916-932
Bracco A, LaCasce J, Pasquero C, Provenzale A. 2000. The velocity distribution of
barotropic turbulence. Phys. Fluids. 12:2478-2488
Brand J, Wouterloot JGA, Rudolph AL, deGeus EJ. 2001. Clumpy outer Galaxy
molecular clouds and the steepening of the IMF. A&A. 377:644-671
Brandenburg A, Zweibel EG. 1994. The formation of sharp structures by ambipolar
diffusion. ApJ. 427:L91-L94
Brandenberg A, Nordlund A, Stein RF, Torkelsson I. 1996. The Disk Accretion Rate for
Dynamo-generated Turbulence. ApJ. 458:L45-L48
Brunt CM, Heyer MH. 2002. Interstellar Turbulence. II. Energy Spectra of Molecular
Regions in the Outer Galaxy. ApJ. 566:289-301
Brunt CM, Heyer MH, Vazquez-Semadeni E, Pichardo B. 2003. Intrinsic, observed and
retrieved properties of interstellar turbulence. ApJ. 595:824-841
Burkert A, Bodenheimer P. 2000. Turbulent molecular cloud cores: Rotational Properties.
ApJ. 543:822-830
Burton WB. 1971. Galactic Structure Derived from Neutral Hydrogen Observations
Using Kinematic Models Based on the Density-wave Theory. A&A. 10:76-96
Bunner AN, Coleman PL, Kraushaar WL, McCammon D. 1971. Low-Energy Diffuse XRays. ApJ. 167:L3-L8
Cambresy L. 1999. Mapping of the extinction in giant molecular clouds using optical star
counts. A&A. 345:965-976
Caselli P. Walmsley CM, Zucconi A, Tafalla M, Dore L, Myers PC. 2002. Molecular
Ions in L1544. I. Kinematics. ApJ. 565:331-343
Castaing B, Gagne Y, Hopfinger EJ 1990. Velocity probability density functions of high
Reynolds number turbulence. Physica D. 46:177-200
Chabrier G. 2003. Galactic Stellar and Substellar Initial Mass Function. PASP.
115:763-795
Chandran BDG. 2003. A review of the theory of incompressible MHD turbulence In
International Workshop on magnetic fields and star formation: theory versus
observations. Dordrecht: Kluwer.
Chandrasekhar S, Munch G. 1952. The Theory of the Fluctuations in Brightness of the
Milky way. V. ApJ. 115:103-123
Chappell D, Scalo J. 2001. Multifractal Scaling, Geometrical Diversity, and Hierarchical
Structure in the Cool Interstellar Medium. ApJ. 551:712-729
Chavanis PH. 2002. Gravitational instability of finite isothermal spheres. A&A .
381:340-356
Chen H, Chen S, Kraichnan RH. 1989. Probability distribution of a statistically advected
scalar field. Phys. Rev. Lett. 63:2657-2660
Chen H, Herring JR, Kerr RM, Kraichnan RH. 1989. Non-Gaussian statistics in isotropic
turbulence. Phys. Fluids A. 1:1844-1854
Chen J-Y, Kollman W. 1994. In Turbulent Reacting Flows. ed. PA Libby, FA Williams.
pp. 211-308. New York:Springer-Verlag. 474 pp.
Chen H, Kandasamy S, Orszag S, Shock R, Succi S, Yakhot V. 2003. Extended
Boltzmann kinetic equation for turbulent flows. Science 301:633-636
Chen Q, Chen S, Eyink GL 2003. The joint cascade of energy and helicity in threedimensional turbulence. Phys. Fluids. 15:361-374
Chen S, Doolen G, Herring JR, Kraichnan RH, Orszag SA, She ZS. 1993. Far dissipation
range of turbulence. Phys. Rev. Lett. 70:3051-3054
Chen S, Kraichnan RH. 1997. Inhibition of turbulent cascade by sweep. J. Plasma Phys.
57:187-193
Chen S, Ecke RE, Eyink GL, Wang X, Xiao Z. 2003. Physical Mechanism of the TwoDimensional Enstrophy Cascade. Phys. Rev. Letts. 91:214501-214501-4
Chew GF, Goldberger ML, Low FE. 1956. The Boltzmann equation and the one-fluid
hydromagnetic equations in the absence of particle collisions. Proc. Roy. Soc. (London)
A 236:112-118
Chiang W-H, Prendergast KH. 1985. Numerical study of a two-fluid hydrodynamic
model of the interstellar medium and population I stars. ApJ. 297:507-530
Chiang W-H. Bregman JN. 1988. A model for the interaction between stars and gas in the
interstellar medium. ApJ. 328:427-439
Cho J, Lazarian A, Vishniac ET. 2002a. Simulations of Magnetohydrodynamic
Turbulence in a Strongly Magnetized Medium. ApJ. 564:291-301
Cho J, Lazarian A, Vishniac ET. 2002b. New Regime of Magnetohydrodynamic
Turbulence: Cascade below the Viscous Cutoff. ApJ. 566:L49-L52
Cho J, Lazarian A. 2002a. Magnetohydrodynamic Turbulence as a Foreground for
Cosmic Microwave Background Studies. ApJ. 575:L63-L66
Cho J, Lazarian A. 2002b. Compressible Sub-Alfvenic MHD Turbulence in Low-
Plasmas. Phys.Rev.Letts. 88:245001-245001-4
Cho J, Lazarian A. 2003c. Compressible Magnetohydrodynamic Turbulence: mode
coupling, scaling relations, anisotropy, new regime and astrophysical implications.
MNRAS. 345:325-339
Cho J, Lazarian A, Vishniac ET. 2003a. MHD turbulence: scaling laws and astrophysical
implications. In Turbulence and magnetic fields in astrophysics. ed. T Passot, E
Falgarone. Springer lecture notes in physics 614:56-100
Cho J, Lazarian A, Vishniac ET. 2003b. Ordinary and Viscosity-damped
Magnetohydrodynamic Turbulence. ApJ. 595:812-823
Christensson M, Hindmarsh M, Brandenburg A. 2001. Inverse cascade in decaying threedimensional magnetohydrodynamic turbulence. Phys Rev E. 64:056405-056405-6
Connaughton C, Nazarenko S, Newell AC. 2003. Dimensional analysis and weak
turbulence. Physica D. 184:86-97
Court A. 1965. Undulence and turbulence. Quart. J. Roy. Meteor. Soc. 91:234-235
Clark BG. 1965. An Interferometer Investigation of the 21-centimeter Hydrogen-Line
Absorption. ApJ. 142:1398-1422
Crovisier J, Dickey JM. 1983. The spatial power spectrum of galactic neutral hydrogen
from observations of the 21-cm emission line. A&A. 122:282-296
Crutcher RM. 1999. Magnetic fields in molecular clouds: observations confront theory.
ApJ. 520:706-713
Dame T, Elmegreen BG, Cohen R, Thaddeus P. 1986. The largest molecular cloud
complexes in the first galactic quadrant. ApJ. 305:892-908
de Avillez MA. 2000. Disc-halo interaction - I. Three-dimensional evolution of the
Galactic disc. MNRAS. 315:479-497
de Avillez MA, Berry DL. 2001. Three-dimensional evolution of worms and chimneys in
the Galactic disc. MNRAS. 328:708-718
de Avillez MA, Breitschwerdt D. 2003a. High resolution simulations of the global and
local ISM. In Star Formation through Time. ASP Conf. Series. ed. Perez, Gonzalez
Delgado, Tenorio-Tagle (astro-ph/0303322)
de Avillez MA, Breitschwerdt D. 2003b. From Large to Small Scales: Global Models of
the ISM. astro-ph/0310633
Delgado-Donate EJ, Clarke CJ, Bate MR. 2003. The dependence of the sub-stellar IMF
on the initial conditions for star formation. MNRAS , in press (astro-ph/0310406)
Deiss BM, Just A, Kegel WH. 1990. Fluctuations of the interstellar medium induced by
the stellar system: mechanical heating and dynamical friction. A&A. 240:123-136
Deshpande AA, Dwarakanath KS, Goss WM 2000. Power Spectrum of the Density of
Cold Atomic Gas in the Galaxy toward Cassiopeia A and Cygnus. ApJ. 543:227-234
Dewan EM. 1985. On the nature of atmospheric waves and turbulence. Radio Sci.
20:1301-1307
Dickey JM. 1985. Small-scale structure and motions in the interstellar gas. In The Milky
Way Galaxy. ed. H van Woerden, RJ Allen, WB Burton. pp. 311-317. Dordrecht: Reidel.
Dickey JM, Salpeter EE, Terzian, Y 1977, Temperature distribution of neutral hydrogen
at high galactic latitudes. ApJ. 211:L77-L82
Dickey JM, Lockman FJ. 1990. H I in the Galaxy. ARAA. 28:215-261
Dickey JM, McClure-Griffiths NM, Stanimirovic S, Gaensler BM, Green AJ. 2001.
Southern Galactic Plane Survey Measurements of the Spatial Power Spectrum of
Interstellar H I in the Inner Galaxy. ApJ. 561:264-271
Dickman RL. 1985. Turbulence in molecular clouds. In Protostars and planets II. ed. DC
Black, MS Matthews. pp. 150-174. Tucson:Univ. Ariz. Press
Dmitruk P, Gomez DO, Matthaeus WH. 2003. Energy spectrum of turbulent fluctuations
in boundary driven reduced magnetohydrodynamics. astroph/0209111
Domaradzki JA, Rogallo RS. 1990. Local energy transfer and nonlocal interactions in
homogeneous, isotropic turbulence. Phys. Fluids A. 2:413-426
Dopazo C. 1994. Recent developments in pdf methods. In Turbulent Reacting Flows, ed.
PA Libby, FA Williams pp. 375-473. New York:Academic Press
Dopazo C, Valino L, Fueyo N. 1997. Statistical description of the turbulent mixing of
scalar fields. Intern. J. Mod. Phys. B. 11:2975-3014
Dubinski J, Narayan R, Phillips TG. 1995. Turbulence in Molecular Clouds. ApJ.
448:226-231
Dubrulle B. 1994. Intermittency in fully developed turbulence: Log-Poisson statistics and
generalized scale covariance. Phys.Rev.Letts. 73:959-962
Elmegreen BG. 1991. The Origin and Evolution of Giant Molecular Clouds. In The
Physics of Star Formation and Early Stellar Evolution. Eds. CJ Lada, ND Kylafis. pp. 3560
Elmegreen BG. 1993. Star Formation at Compressed Interfaces in Turbulent Selfgravitating Clouds. ApJ. 419:L29-L32
Elmegreen BG. 1999. Formation and Loss of Hierarchical Structure in Two-dimensional
Magnetohydrodynamic Simulations of Wave-driven Turbulence in Interstellar Clouds.
ApJ. 527:266-284
Elmegreen BG. 2000. Star Formation in a Crossing Time. ApJ. 530:277-281
Elmegreen BG, Elmegreen DM. 2001. Fractal Structure in Galactic Star Fields. AJ.
121:1507-1511
Elmegreen BG, Kim S, Staveley-Smith L. 2001. A Fractal Analysis of the H I Emission
from the Large Magellanic Cloud. ApJ. 548:749-769
Elmegreen DM, Elmegreen BG, Eberwein KS. 2002. Dusty Acoustic Turbulence in the
Nuclear Disks of Two LINER Galaxies NGC 4450 and NGC 4736. ApJ. 564:234-243
Elmegreen BG, Elmegreen DM, Leitner SN. 2003. A Turbulent Origin for Flocculent
Spiral Structure in Galaxies. ApJ . 590:271-283
Esquivel A, Lazarian A, Pogosyan D, Cho J. 2003. Velocity statistics from spectral line
data: effects of density-velocity correlations, magnetic field and shear. MNRAS.
342:325-336
Falgarone E, Passot, T. eds. 2003. Turbulence and Magnetic Fields in Astrophysics,
Springer Lecture Notes Phys., 614
Falgarone E, Phillips TG. 1990. A signature of the intermittency of interstellar turbulence
- The wings of molecular line profiles. ApJ. 359:344-354
Falgarone E, Phillips TG, Walker CK. 1991. The edges of molecular clouds - Fractal
boundaries and density structure. ApJ. 378:186-201
Falgarone E, Puget JL, Perault M. 1992. A&A. The small-scale density and velocity
structure of quiescent molecular clouds 257:715-730
Falgarone E, Lis DC, Phillips TG, Pouquet A, Porter DH, Woodward PR. 1994.
Synthesized spectra of turbulent clouds. ApJ. 436:728-740
Falgarone E, Panis J-F, Heithausen A, Perault M, Stutzki J, Puget J-L, Bensch F. 1998.
The IRAM key-project: small-scale structure of pre-star-forming regions. I.
Observational results. A&A. 331:669-696
Falgarone E, Pety J, Phillips TG. 2001. Filamentary Structure and Helical Magnetic
Fields in the Environment of a Starless Dense Core. ApJ. 555:178-190
Falgarone E, Hily-Blant P, Levrier F. 2003. Structure of molecular clouds. In Magnetic
Fields and Star Formation: theory versus observations. Eds. AI Gomez de Castro et al.
Dordrecht:Kluwer, in press
Falgarone E, Verstraete L, Pineau des Forets G, Hily-Blant P. 2004. Warm gas in the cold
diffuse interstellar medium: spectral signatures in the H2 pure rotational lines. A&A. , in
press.
Fatuzzo M, Adams FC. 2002. Enhancement of Ambipolar Diffusion Rates through Field
Fluctuations. ApJ. 570:210-221
Ferriere KM, Zweibel EG, Shull JM. 1988. Hydromagnetic wave heating of the lowdensity interstellar medium. ApJ . 332:984-994
Field GB, Goldsmith DW, Habing HJ. 1969. Cosmic-Ray Heating of the Interstellar Gas.
ApJ. 155:L149-L154
Fisher RT. 2003. A Turbulent Interstellar Medium Origin of the Binary Period
Distribution. astro-ph/0303280
Fleck RC Jr. 1981. On the generation and maintenance of turbulence in the interstellar
medium. ApJ . 246:L151-L154
Frisch U. 1995. Turbulence. Cambridge: Cambridge Univ. Press. pp. 296
Fosalba P, Lazarian A, Prunet S, Tauber JA. 2002. Statistical Properties of Galactic
Starlight Polarization. ApJ. 564:762-772
Franco J, Carraminana A. (eds.). 1999. Interstellar Turbulence. Cambridge: Cambridge
Univ. Press. 287 pages.
Fuchs B, von Linden S. 1998. Dynamical stability and evolution of the discs of SC
galaxies. MNRAS . 294:513-522
Fukunaga M, Tosa M. 1989. N-body simulation of giant molecular clouds in a galaxy. II
- Viscous heating of giant molecular cloud gas and effects of inelastic collisions. PASJ .
41:241-262
Galtier S. 2003. Weak inertial-wave turbulence theory. Phys. Rev. E. 68:015301-1015301-4
Galtier S, Nazarenko SV, Newell AC, Pouquet A. 2000. A weak turbulence theory for
incompressible magnetohydrodynamics. J. Plasma Physics. 63:447-488
Galtier S, Nazarenko SV, Newell AC, Pouquet A. 2002. Anisotropic turbulence of shearAlfven waves. ApJ. 564:L49-L52
Gammie, CF 2001, Nonlinear Outcome of Gravitational Instability in Cooling, Gaseous
Disks, ApJ , 553, 174
Gammie CF, Ostriker JP, Jog CJ. 1991, The velocity dispersion of giant molecular
clouds. II - Mathematical and numerical refinements. ApJ . 378:565-575
Gammie CF, Lin Y-T, Stone JM, Ostriker EC. 2003. Analysis of Clumps in Molecular
Cloud Models: Mass Spectrum, Shapes, Alignment, and Rotation. ApJ. 592:203-216
Gaustad JE, VanBuren D. 1993. The distribution of interstellar dust in the solar
neighborhood. PASP. 105:1127-1140
Gautier TN, Boulanger F, Perault M, Puget JL. 1992. A calculation of confusion noise
due to infrared cirrus. AJ. 103:1313-1324
Gazol-Patino A, Passot T. 1999. A Turbulent Model for the Interstellar Medium. III.
Stratification and Supernova Explosions. ApJ. 518:748-759
Gazol A, Vazquez-Semadeni E, Sanchez-Salcedo FJ, Scalo J. 2001. The Temperature
Distribution in Turbulent Interstellar Gas. ApJ. 557:L121-L124
Gerola H, Kafatos M, McCray R. 1974. Statistical Time-Dependent Model for the
Interstellar Gas. ApJ. 189:55-66
Gill AG, Henriksen RN. 1990. A first use of wavelet analysis for molecular clouds. ApJ.
365:L27-L30
Goldman I. 2000. Interpretation of the Spatial Power Spectra of Neutral Hydrogen in the
Galaxy and in the Small Magellanic Cloud ApJ. 541:701-706
Goldreich P, Kwan J. 1974. Molecular Clouds. ApJ. 189:441-454
Goldreich P, Sridhar S. 1995. Toward a theory of interstellar turbulence. 2: Strong
Alfvenic turbulence. ApJ. 438:763-775
Goldreich P, Sridhar S. 1997. Magnetohydrodynamic Turbulence Revisited. ApJ.
485:680-688
Goodman AA, Bastien P, Menard F, Myers PC. 1990. Optical polarization maps of starforming regions in Perseus, Taurus, and Ophiuchus. ApJ. 359:363-377
Goodman AA, Benson PJ, Fuller GA, Myers PC. 1993. Dense cores in dark clouds. VIII
- Velocity gradients. ApJ. 406:528-547
Goodwin SP, Whitworth AP, Ward-Thompson D. 2003. Simulating star formation in
molecular cloud cores I. The influence of low levels of turbulence on fragmentation and
multiplicity. A&A. in press (astro-ph/0309829)
Gotoh T, Kraichnan RH. 1993. Statistics of decaying Burgers turbulence. Phys. Fluids
A. 5:445-457
Grant HL, Stewart RW, Moillet A, 1962. Turbulence spectra from a tidal channel. J.
Fluid Mech. 12:241-268
Green DA. 1993. Power spectrum analysis of the angular scale of Galactic neutral
hydrogen emission towards L = 140 deg, B = 0 deg. MNRAS. 262:327-342
Hall AN. 1980. On the origin of long time-scale pulsar scintillations - I. cosmic ray
streaming or the mirror instability? MNRAS. 190:353-369
Hartmann L, Ballesteros-Paredes J, Bergin EA. 2001. Rapid Formation of Molecular
Clouds and Stars in the Solar Neighborhood. ApJ. 562:852-868
Hasegawa A. 1985. Self-organization processes in continuous media. Advances in Phys.
34:1-42.
Hatakeyama N, Kambe T. 1997. Statistical Laws of Random Strained Vortices in
Turbulence. Phys.Rev.Letts. 79:1257-1260
Haugen NEL, Brandenburg A, Dobler W. 2003. Simulations of nonhelical hydromagnetic
turbulence. ApJ. 597: L141-44
Heiles C. 1970. Motions and Physical Conditions Inside Dust Clouds. ApJ. 160:51-58
Heiles C, Goodman AA, McKee CF, Zweibel EG. 1993. Magnetic fields in star-forming
regions--Observations. In Protostars and Planets III, ed. EH Levy, JI Lunine. pp. 279326. Tucson:Univ. of Arizona.
Heiles C. 2001. New temperatures of diffuse interstellar gas: Thermally unstable gas.
ApJ. 551:L105-L108
Heithausen A. 1996. On the dynamical state of high-latitude molecular clouds. A&A.
314:251-257
Heitsch F, Mac Low M-M, Klessen RS. 2001. Gravitational Collapse in Turbulent
Molecular Clouds. II. Magnetohydrodynamical Turbulence. ApJ. 547:280-291
Heitsch F, Zweibel EG, Slyz AD, Devriendt JEG. 2003. Turbulent Ambipolar Diffusion:
Numerical Studies in 2D. astroph/0309306, preprint (ApJ in press)
Hetem A Jr, Lepine JRD. 1993. Fractal 3-D simulations of molecular clouds. A&A.
270:451-461
Heyer MH, Schloerb FP. 1997. Application of Principal Component Analysis to LargeScale Spectral Line Imaging Studies of the Interstellar Medium. ApJ. 475:173-187
Heyer MH, Brunt C, Snell RL, Howe JE, Schloerb FP, Carpenter JM. 1998. The Five
College Radio Astronomy Observatory CO Survey of the Outer Galaxy. ApJS.
115:241-258
Heyer MH, Carpenter JM, Snell RL. 2001. The Equilibrium State of Molecular Regions
in the Outer Galaxy. ApJ. 551:852-866
Higdon JC. 1986. Density fluctuations in the interstellar medium: Evidence for
anisotropic magnetogasdynamic turbulence. II - Stationary structures. ApJ. 309:342361
Hinze, JO. 1975. Turbulence, 2nd Ed. New York:McGraw-Hill. pp. 790.
Hobbs LM. 1974. Statistical properties of interstellar clouds. ApJ. 191:395-399
Hobson MP. 1992. High-resolution HCO(+) and HCN observations of M17SW Clumps, turbulence and cloud support. MNRAS. 256:457-476
Houde M, Bastien P, Dotson JL, Dowell CD, Hildebrand RH, Peng R, Phillips TG,
Vaillancourt JE, Yoshida H. 2002. On the Measurement of the Magnitude and
Orientation of the Magnetic Field in Molecular Clouds. ApJ. 569:803-814
Houlahan P, Scalo J. 1990. Recognition and characterization of hierarchical interstellar
structure. I - Correlation function. ApJS. 72:133-152
Houlahan P, Scalo J. 1992. Recognition and characterization of hierarchical interstellar
structure. II - Structure tree statistics. ApJ. 393:172-187
Huber D, Pfenniger D. 2001. Lumpy structures in self-gravitating disks. A&A .
374:465-493
Huber D, Pfenniger D. 2002. Long-range correlations in self-gravitating N-body systems.
A&A . 386:359-378
Hunter JH Jr, Sandford MT II, Whitaker RW, Klein RI. 1986. Star formation in colliding
gas flows. ApJ. 305:309-332
Ikeuchi S, Spitzer L Jr. 1984. Scattering of shock waves by a spherical cloud. ApJ .
283:825-832
Ingalls JG, Bania TM, Lane AP, Rumitz M, Stark AA. 2000. Physical State of Molecular
Gas in High Galactic Latitude Translucent Clouds. ApJ. 535:211-226
Iroshnikov PS. 1964. Turbulence of a Conducting Fluid in a Strong Magnetic Field.
Sov. Astron. 7:566-571
Jackson T, Werner M, Gautier TN III. 2003. A Catalog of Bright Filamentary Structures
in the Interstellar Medium. ApJS. 149:365-373
Jayesh, Warhaft Z. 1991. Probability distribution of a passive scalar in grid-generated
turbulence. Phys. Rev. Lett. 67:3503-3506
Jenkins JB. 2003. Evidence and Implications of Pressure Fluctuations in the ISM. In
From Observations to Self-Consistent Modelling of the ISM in Galaxies. ed. G Hensler,
G Stasinska, S Harfst, P Kroupa, C Theis. Dordrecht: Kluwer. in press
Jenkins EB, Meloy DA. 1974. A survey with Copernicus of interstellar O VI absorption.
ApJ. 193:L121-L125
Jessop NE, Ward-Thompson D. 2001. The initial conditions of isolated star formation IV. C18O observations and modeling of the pre-stellar core L1689B. MNRAS.
323:1025-1034
Jijina J, Myers PC, Adams FC. 1999. Dense cores mapped in ammonia: A database.
ApJS. 125:161-236
Kaplan SA. 1958. Theory of isotropic magnetic turbulence in gases. In Electromagnetic
phenomena in cosmical physics. Proc. IAU Symp. No. 6. ed. B Lehnert. pp. 504-512.
Cambridge:Cambridge Univ. Press
Kaneda Y. Ishihara T. Yokokawa M. Itakura K. Uno A. 2003. Energy dissipation rate and
energy spectrum in high resolution direct numerical simulations of turbulence in a
periodic box. Physics of Fluids. 15:L21-L24
Kanekar N. Subrahmanyan R. Chengalur JN. Safouris V. 2003. The temperature of the
WNM in the Milky Way. astroph/0310761
Kawamura A, Onishi T, Yonekura Y, Dobashi K, Mizuno A, Ogawa H, Fukui Y. 1998.
A 13CO survey of molecular clouds in Gemini and Auriga. ApJS. 117:387-425
Kegel WH. 1989. The interpretation of correlations between observed parameters of
molecular clouds. A&A. 225:517-520
Kida S, Murakami Y. 1989. Statistics of velocity gradients in turbulence at moderate
Reynolds numbers. Fluid Dyn. Res. 4:347-370
Kim J, Balsara D, Mac Low M-M. 2001. Turbulence Driven by Supernova Explosions in
a Radiatively-Cooling Magnetized Interstellar Medium. J. Korean Astron. Soc. 34:333335
Kim S, Staveley-Smith L, Dopita MA, Freeman KC, Sault RJ, Kesteven MJ, McConnell
D. 1998. An HI aperture synthesis of the Large Magellanic Cloud. ApJ. 503:674-688
Kim S, Staveley-Smith L, Dopita M, Sault RJ, Freeman KC, Lee Y, Chu Y-H. 2003. A
Neutral Hydrogen Survey of the Large Magellanic Cloud: Aperture Synthesis and
Multibeam Data Combined. ApJS. 148:473-486
Kim W-T, Ostriker E, Stone J. 2003. Magnetorotationally-Driven Galactic Turbulence
and the Formation of Giant Molecular Clouds. astroph/039080
Kinney RM, McWilliams JC. 1998. Turbulent cascades in anisotropic
magnetohydrodynamics. Phys. Rev. E. 57:7111ñ7121
Kitamura Y, Sunada K, Hayashi M, Hasegawa T. 1993. High-resolution observations of
turbulence in the subcondensation TMC-1C in Heiles' cloud 2 - Estimation of the velocity
spectrum of turbulence. ApJ. 413:221-236
Klein RI, Woods DT. 1998. Bending Mode Instabilities and Fragmentation in Interstellar
Cloud Collisions: A Mechanism for Complex Structure. ApJ . 497:777-799
Klein RI, Fisher RT, Krumholz MR, McKee CF. 2003. Recent advances in the collapse
and fragmentation of turbulent molecular cloud cores. In Winds, Bubbles & Explosions:
A Conference to Honour John Dyson. ed. SJ Arthur, WJ Henney. Rev. Mex. A&A.
15:92-96
Kleiner SC, Dickman RL. 1985. Large-scale structure of the Taurus molecular complex.
II - Analysis of velocity fluctuations and turbulence. III - Methods for turbulence. ApJ.
295:466-478
Kleiner SC, Dickman RL. 1987. Small-scale structure of the Taurus molecular clouds:
Turbulence in Heiles' Cloud 2. ApJ. 312:837-847
Klessen RS. 2000. One-Point Probability Distribution Functions of Supersonic Turbulent
Flows in Self-gravitating Media. ApJ. 535:869-886
Klessen RS. 2001. The Formation of Stellar Clusters: Mass Spectra from Turbulent
Molecular Cloud Fragmentation. ApJ. 556:837-846
Klessen RS, Burkert A, Bate MR. 1998. Fragmentation of Molecular Clouds: The Initial
Phase of a Stellar Cluster. ApJ. 501:L205-L208
Klessen RS, Burkert A. 2000. The Formation of Stellar Clusters: Gaussian Cloud
Conditions. I. ApJS. 128:287-319
Klessen RS. Burkert A. 2001. The Formation of Stellar Clusters: Gaussian Cloud
Conditions. II. ApJ. 549:386-401
Klessen RS, Heitsch F, Mac Low M-M 2000. Gravitational Collapse in Turbulent
Molecular Clouds. I. Gasdynamical Turbulence. ApJ. 535:887-906
Kolesnik I, Ogul'Chanskii II. 1990. Supersonic turbulent fragmentation of giant
molecular clouds. In Physical processes in fragmentation and star formation, ed. R
Capuzzo-Dolcetta, C Chiosi, A di Fazio, pp. 81-86. Dordrecht: Kluwer
Kolmogorov AN. 1941. The local structure of turbulence in incompressible viscous fluid
for very large Reynolds numbers. reprinted in 1991 Proc. Roy. Soc. London A. 434:913
Kornreich P, Scalo J. 2000. The galactic shock pump: A source of supersonic internal
motions in the cool interstellar medium. ApJ . 531:366-383
Korpi MJ, Brandenburg A, Shukurov A, Tuominen I. 1999a. Evolution of a superbubble
in a turbulent, multi-phased and magnetized ISM. A&A. 350:230-239
Korpi MJ, Brandenburg A, Shukurov A, Tuominen I, Nordlund A. 1999b. A Supernovaregulated Interstellar Medium: Simulations of the Turbulent Multiphase Medium. ApJ.
514:L99-L102
Kraichnan RH. 1965. Inertial-range spectrum of hydrodynamic turbulence. Phys. Fluids.
8:1385-1387
Kraichnan RH. 1967. Inertial ranges in two-dimensional turbulence. Phys. Fluids.
10:1417-1423
Kritsuk AG, Norman ML. 2002a. Interstellar Phase Transitions Stimulated by Timedependent Heating. ApJ. 580:L51-L55
Kritsuk AG, Norman ML. 2002b. Thermal Instability-induced Interstellar Turbulence
2002. ApJ. 569:L127-L131
Kritsuk AG, Norman ML. 2003. Scaling relations for turbulence in multiphase interstellar
medium. astroph/0310697
Kudoh T. Basu S. 2003. Nonlinear Hydromagnetic Wave Support of a Stratified
Molecular Cloud. ApJ. 595:842-857
Kulkarni SR, Heiles C. 1988. Neutral hydrogen and the diffuse interstellar medium. In
Galactic and extragalactic radio astronomy. ed. GL Verschuur, KI Kellerman, pp. 95-153.
New York: Springer-Verlag
Kulsrud RM. 1983. MHD description of plasma. In Basic Plasma Physics, Vol 1. eds. AA
Galeev, RN Sudan. pp. 115-145
Kurien S, Taylor MA, Matsumoto T. 2003. Cascade time-scales for energy and helicity in
homogeneous isotropic turbulence. ADS arxiv.org nlin.CD/0312034.
Langer WD, Wilson RW, Anderson CH. 1993. Hierarchical structure analysis of
interstellar clouds using nonorthogonal wavelets. ApJ. 408:L45-L48
Langer WD, Velusamy T, Kuiper TBH, Levin S, Olsen E, Migenes V. 1995. Study of
Structure and Small-Scale Fragmentation in TMC-1. ApJ. 453:293-307
Larson RB. 1981. Turbulence and star formation in molecular clouds. MNRAS.
194:809-826
Laveder D, Passot T, Sulem PL. 2001. Transverse collapse of low-frequency Alfven
waves. Physica D. 152-153:694-704
Laveder D, Passot T, Sulem PL. 2002. Transverse dynamics of dispersive Alfven waves.
I. Direct numerical evidence of filamentation. Phys. of Plasmas. 9:293-304
Lazarian A. 1999, Statistics of Turbulence from Spectral-Line Data Cubes. In Plasma
Turbulence and Energetic Particles in Astrophysics. ed. M Ostrowski, R Schlickeiser. pp.
28-47. Krakow:Obserwatorium Astronomiczne Uniwersytet Jagiellonski.
Lazarian A, Pogosyan D. 2000. Velocity Modification of H I Power Spectrum. ApJ.
537:720-748
Lazarian A, Pogosyan D, Vazquez-Semadeni E, Pichardo B. 2001. Emissivity Statistics
in Turbulent Compressible Magnetohydrodynamic Flows and the Density-Velocity
Correlation. ApJ. 555:130-138
Lazarian A, Esquivel A. 2003. Statistics of Velocity from Spectral Data: Modified
Velocity Centroids. ApJ. 592:L37-L40
Lazarian A, Vishniac ET, Cho J. 2003. Magnetic field structure and stochastic
reconnection in a partially ionized gas. astroph/0311051
Lee H, Ryu D, Kim J, Jones TW, Balsara D. 2003. Numerical study of compressible
magnetohydrodynamic turbulence in two dimensions. ApJ. 594:627-636.
Lele SK. 1994. Compressibility effects on turbulence. Ann. Rev. Fluid Mech. 26:211254
Lelong M-P, Riley JJ. 1991. Internal wave-vortical mode interactions in strongly
stratified flows. J. Fluid Mech. 232:1-19
Leorat J, Passot T, Pouquet A. 1990. Influence of supersonic turbulence on selfgravitating flows. MNRAS. 243:293-311
Lesieur M. 1990. Turbulence in Fluids: Stochastic and Numerical Modeling. Dordrecht:
Kluwer. 412 pp.
Leslie DC. 1973. Developments in the Theory of Turbulence. Oxford: Clarendon. 368 pp.
Levy EH, Lunine JI. Eds. 1993 Protostars and Planets III. Tucson: Univ. Ariz. Press
Li Y, Klessen RS, Mac Low M-M. 2003. The Formation of Stellar Clusters in Turbulent
Molecular Clouds: Effects of the Equation of State. ApJ. 592:975-985
Li PS, Norman ML, Mac Low M-M, Heitsch F. 2003. The Formation of Self-Gravitating
Cores in Turbulent Magnetized Clouds. astro-ph/0312622
Lis DC, Pety J, Philips TG, Falgarone E. 1996. Statistical Properties of Line Centroid
Velocities and Centroid Velocity Increments in Compressible Turbulence. ApJ .
463:623-629
Lis DC, Keene J, Li Y, Phillips TG, Pety J. 1998. Statistical Properties of Line Centroid
Velocity Increments in the rho Ophiuchi Cloud. ApJ . 504:889-899
Liszt HS, Wilson RW, Penzias AA, Jefferts KB, Wannier PG, Solomon PM. 1974. CO
and CS in the Orion Nebula. ApJ. 190:557-564
Lithwick Y, Goldreich P. 2001. Compressible Magnetohydrodynamic Turbulence in
Interstellar Plasmas. ApJ. 562: 279-296
Lithwick Y, Goldreich P. 2003. Imbalanced Weak Magnetohydrodynamic Turbulence.
ApJ. 582:1220-1240
Little LT, Matheson DN. 1973. Radio scintillations due to plasma irregularities with
power law spectra: the interstellar medium. 1973. MNRAS. 162:329-338
Liu L, She Z-S. 2003. Hierarchical structure description of intermittent structures of
turbulence. Fluid Dyn. Res. 33:261-286
Loren RB. 1989. The cobwebs of Ophiuchus. I - Strands of (C-13)O - The mass
distribution. ApJ. 338:902-924
Low FJ, Young E, Beintema DA, Gautier TN, Beichman CA, Aumann HH, Gillett FC,
Neugebauer G, Boggess N, Emerson JP. 1984. Infrared cirrus - New components of the
extended infrared emission. ApJ. 278:L19-L22
Lundgren TS. 1982. Strained spiral vortex model for turbulent fine structure. Phys.
Fluids. 25:2193-2203
L'vov VS. L'vov YuV. Pomyalov A. 2000. Anisotropic spectra of acoustic turbulence.
Phys. Rev. E 61:2586-2594
Mac Low M-M. 1999. The Energy Dissipation Rate of Supersonic,
Magnetohydrodynamic Turbulence in Molecular Clouds. ApJ. 524:169-178
Mac Low M-M. 2003. MHD turbulence in star-forming regions and the interstellar
medium. In Simulations of magnetohydrodynamic turbulence in astrophysics, ed. T
Passot, E Falgarone. Springer Lecture Notes in Physics. pp. 182-212
Mac Low M-M, Norman ML. 1993. Nonlinear growth of dynamical overstabilities in
blast waves. ApJ. 407:207-218
Mac Low M-M, Norman ML, Konigl A, Wardle M. 1995. Incorporation of ambipolar
diffusion into the ZEUS magetohydrodynamics code. ApJ. 442:726-735
Mac Low M-M, Klessen RS, Burkert A, Smith MD 1998. Kinetic Energy Decay Rates of
Supersonic and Super-Alfvenic Turbulence in Star-Forming Clouds. Phys. Rev. Lett.
80:2754-2757
Mac Low M-M, Klessen RS. 2004. Control of star formation by supersonic turbulence.
Rev. Mod. Phys. in press (astroph/031093)
Maron J, Goldreich P. 2001. Simulations of incompressible magnetohydrodynamic
turbulence. ApJ. 554:1175-1196
Martos MA, Cox DP. 1998. Magnetohydrodynamic Modeling of a Galactic Spiral Arm
as a Combination Shock and Hydraulic Jump. ApJ . 509:703-716
Mathieu J, Scott J. 2000. An introduction to turbulent flow. Cambridge: Cambridge Univ.
Press pp. 374
Matthaeus WH, Bieber JW, Zank GP. 1995. Unquiet on any front: Anisotropic turbulence
in the solar wind. Rev. Geophys. Suppl. 33:609-614
Matthaeus WM, Oughton S, Ghosh S, Hossain M. 1998. Scaling of Anisotropy in
Hydromagnetic Turbulence. Phys. Rev. Lett. . 81:2056-2059
McComb WD. 1990. Physics of Fluid Turbulence. Oxford: Oxford Univ. Press. pp. 572
McCray R, Snow TP Jr. 1979. The violent interstellar medium. ARAA. 17:213-240
McGee RX, Milton JA, Wolfe W. 1966. A Sky Survey of Neutral Hydrogen at lambda 21
cm. Aust. J. Phys. Suppl. 1:3-39
McKee CF, Ostriker JP. 1977. A theory of the interstellar medium - Three components
regulated by supernova explosions in an inhomogeneous substrate. ApJ. 218:148-169
McKee C, Zweibel EG. 1992. On the virial theorem for turbulent molecular clouds.
ApJ. 399:551-562
Mebold U, Hachenberg O, Laury-Micoulaut CA. 1974. A Statistical Model for the
Intercloud HI-Gas. I. Theory. A&A. 30:329-338
Miesch MS, Bally J. 1994. Statistical analysis of turbulence in molecular clouds. ApJ.
429:645-671
Miesch MS, Zweibel EG. 1994. Shock propagation and the generation of
magnetohydrodynamic wave fields in inhomogeneous molecular clouds. ApJ . 432:622640
Miesch MS, Scalo JM. 1995. Exponential Tails in the Centroid Velocity Distributions of
Star-Forming Regions. ApJ . 450:L27-L30
Miesch MS, Scalo J, Bally J. 1999. Velocity Field Statistics in Star-forming Regions. I.
Centroid Velocity Observations. ApJ. 524:895-922
Minkowski R. 1955. The observational background of cosmical gasdynamics. In Gas
Dynamics of Cosmic Clouds. ed. JM Burgers, HC van de Hulst. pp. 3-12. Amsterdam:
North Holland
Miville-Deschenes M -A, Joncas G, Falgarone E. 1999. Turbulence in the Ursa Major
cirrus cloud. In Interstellar Turbulence, ed. J Franco, A Carraminana (Cambridge:
Cambridge Univ. Press). pp. 169-173.
Miville-Deschenes M-A, Levrier F, Falgarone E. 2003. On the Use of Fractional
Brownian Motion Simulations to Determine the Three-dimensional Statistical Properties
of Interstellar Gas. ApJ. 593:831-847
Moisy F, Tabeling P, Willaime H. 1999. Kolmogorov equation in a fully developed
turbulence experiment. Phys. Rev. Lett. 82:3994-3997
Monin AS, Yaglom AM. 1975. Statistical Fluid Mechanics: Mechanics of Turbulence.
Cambridge: MIT Press. ed. J Lumley. 2 vol. 873 pp.
Montgomery D, Matthaeus WH. 1995. Anisotropic modal energy transfer in interstellar
turbulence. ApJ. 447:706:707
Mouri H., Takaoka M, Hori A, Kawashima Y. 2003. Probability density function of
turbulent velocity fluctuations in a rough-wall boundary layer. Phys. Rev. E.
68:036311-1-036311-6
Mouschovias TC, Paleologou EV. 1979. The angular momentum problem and magnetic
braking - an exact time-dependent solution. ApJ. 230:204-222
Mouschovias TC 1991. Magnetic braking, ambipolar diffusion, cloud cores, and star
formation - Natural length scales and protostellar masses. ApJ. 373:169-186
Muller W-C, Biskamp D. 2000. Scaling properties of three dimensional
magnetohydrodynamical turbulence. Phys. Rev. Lett. 84:475-478
Muller W-C, Biskamp D, Grappin R. 2003. Statistical anisotropy of
magnetohydrodynamic turbulence. Phys. Rev. E. 67:066302-1-066302-4
Muller W-C, Biskamp D. 2003. The evolving phenomenological view on
magnetohydrodynamic turbulence. In Turbulence and magnetic fields in astrophysics,
eds. E Falgarone, T Passot, NY: Springer. Lecture Notes in Physics 614, 462pp, 3-27
Myers PC. 1983. Dense cores in dark clouds. III - Subsonic turbulence. ApJ. 270:105118
Myers PC, Fuller GA, Goodman AA, Benson PJ. 1991. Dense cores in dark clouds. VI Shapes. ApJ. 376:561-572
Nakayama K. 2002. Lagrangian Statistical Theory of Anisotropic MHD Turbulence.
PASJ. 54:1065-1078
Ng CS, Bhattacharjee A. 1996. Interaction of shear-Alfven wave packets: implication for
weak magnetohydrodynamic turbulence in astrophysical plasmas. ApJ. 465:845-854
Ng CS, Bhattacharjee A. 1997. Scaling of anisotropic spectra due to the weak interaction
of shear-Alfven wave packets. Phys. of Plasmas. 4:605-610
Nordlund A, Padoan P. 1999. The Density PDFs of Supersonic Random Flows. In
Interstellar Turbulence, Proceedings of the 2nd Guillermo Haro Conference. ed. J Franco,
A Carraminana. pp. 218-222. Cambridge: Cambridge Univ. Press.
Nordlund A, Padoan P. 2003. Star Formation and the Initial Mass Function. In
Simulations of Magnetohydrodynamic Turbulence in Astrophysics: Recent
Achievements and Perspectives. ed. E Falgarone, T Passot, Lecture Notes in Physics.
614:271-298
Norman CA, Ferrara A. 1996. The turbulent interstellar medium: generalizing to a scaledependent phase continuum. ApJ . 467:280-291
Noullez A, Wallace G, Lempert W, Miles RB, Frisch U 1997. Transverse velocity
increments in turbulent flow using the relief technique. J. Fluid Mech. 339:287-307
Oey MS, Clarke CJ. 1997. The superbubble size distribution in the interstellar medium of
galaxies. MNRAS . 289:570-588
Oort JH, Spitzer L Jr. 1955. Acceleration of Interstellar Clouds by O-Type Stars. ApJ.
121:6-23
Ossenkopf V. 2002. Molecular line emission from turbulent molecular clouds. A&A.
391:295-315
Ossenkopf V, Klessen RS, Heitsch F. 2001. On the structure of self-gravitating molecular
clouds. A&A. 379:1005-1016
Ossenkopf V, Mac Low M-M. 2002. Turbulent velocity structure in molecular clouds.
A&A. 390:307-326
Ostriker EC. 2003. Developing diagnostics of molecular clouds using numerical MHD
simulations. in Simulations of magnetohydrodynamic turbulence in astrophysics, ed. T
Passot, E Falgarone. Springer Lecture Notes in Physics. pp. 252-270. astro-ph/0204463
Ostriker EC, Gammie CF, Stone JM. 1999. Kinetic and Structural Evolution of Selfgravitating, Magnetized Clouds: 2.5-dimensional Simulations of Decaying Turbulence.
ApJ. 513:259-274
Ostriker EC, Stone JM, Gammie, CF 2001. Density, Velocity, and Magnetic Field
Structure in Turbulent Molecular Cloud Models. ApJ. 546:980-1005
Ottino JM. 1989. The Kinematics of Mixing: Stretching, Chaos and Transport.
Cambridge:Cambridge Univ. Press. pp. 364
Padoan P, Jones BJT, Nordlund A. 1997. Supersonic Turbulence in the Interstellar
Medium: Stellar Extinction Determinations as Probes of the Structure and Dynamics of
Dark Clouds. ApJ. 474:730-734
Padoan P, Juvela M, Bally J, Nordlund A. 1998. Synthetic Molecular Clouds from
Supersonic Magnetohydrodynamic and Non-LTE Radiative Transfer Calculations. ApJ.
504:300-313
Padoan P, Bally J, Billawala Y, Juvela M, Nordlund A. 1999. Supersonic turbulence in
the Perseus molecular cloud. ApJ. 525:318-329
Padoan P, Nordlund A. 1999. A super-Alfvenic model of dark clouds. ApJ. 526:279294
Padoan P, Juvela M, Bally J, Nordlund A. 2000. A Comparison of 13CO Local
Thermodynamic Equilibrium and True Column Densities in Molecular Cloud Models.
ApJ. 529:259-267
Padoan P, Zweibel EG, Nordlund A. 2000. Ambipolar Drift Heating in Turbulent
Molecular Clouds. ApJ. 540:332-341
Padoan P. Juvela M. Goodman AA. Nordlund A. 2001b. The Turbulent Shock Origin of
Proto-Stellar Cores. ApJ. 553:227-234
Padoan P, Kim S, Goodman A, Staveley-Smith L. 2001c. A New Method to Measure and
Map the Gas Scale Height of Disk Galaxies. ApJ. 555:L33-L36.
Padoan P, Cambresy L, Langer W. 2002. Structure Function Scaling of a 2MASS
Extinction Map of Taurus. ApJ. 580:L57-L60
Padoan P, Goodman AA, Juvela M. 2003. The Spectral Correlation Function of
Molecular Clouds: A Statistical Test for Theoretical Models. ApJ. 588:881-893
Padoan P, Boldyrev S, Langer W, Nordlund A. 2003a. Structure Function Scaling in the
Taurus and Perseus Molecular Cloud Complexes. ApJ. 583:308-313
Padoan P, Jimenez R, Nordlund A, Boldyrev S. 2003b. Structure function scaling in
compressible super-Alfvenic MHD turbulence. astro-ph/0301026.
Park Y-S, Hong SS, Minh YC. 1996. Excitations and line profiles of CO in clumpy
molecular clouds: radiative interactions of clump and interclump media. A&A.
312:981-988
Parravano A, Hollenbach DJ, McKee CF. 2003. Time Dependence of the Ultraviolet
Radiation Field in the Local Interstellar Medium. ApJ. 584:797-817
Passot T, Pouquet A, Woodward P. 1988. The plausibility of Kolmogorov-type spectra in
molecular clouds. A&A. 197:228-234
Passot T, Vazquez-Semadeni E, Pouquet A 1995. A Turbulent Model for the Interstellar
Medium. II. Magnetic Fields and Rotation. ApJ. 455:536-555
Passot T, Vazquez-Semadeni E. 1998. Density probability distribution in onedimensional polytropic gas dynamics. Phys. Rev. 58:4501-4510
Passot T, Sulem PL. 2003a. Long-Alfven-wave trains in collisionless plasmas. I. Kinetic
theory. Phys.Plasmas. 10:3887-3905
Passot T, Sulem PL. 2003b. Filamentation instability of long Alfven waves in warm
collisionless plasmas. Phys.Plasmas. 10:3914-3921
Passot T, Vazquez-Semadeni E. 2003. The correlation between magnetic pressure and
density in compressible MHD turbulence. A&A. 398:845-855
Pavlovski G, Smith MD, Mac Low M-M, Rosen A. 2002. Hydrodynamical simulations
of the decay of high-speed molecular turbulence - I. Dense molecular regions. MNRAS.
337: 477-487
Peng R, Langer WD, Velusamy T, Kuiper TBH, Levin S. 1998. Low-mass clumps in
TMC-1: Scaling laws in the small scale regime. ApJ. 497:842-849
Perault M, Falgarone E, Puget JL. 1986. Fragmented molecular clouds - Statistical
analysis of the C-13O (J = 1 - 0) emission distribution. A&A. 157:139-147
Pety J, Falgarone E. 2000. The Elusive Structure of the Diffuse Molecular Gas: Shocks or
Vortices in Compressible Turbulence? A&A . 356:279-286
Pety J, Falgarone E. 2003. Non-Gaussian velocity shears in the environment of low mass
dense cores. A&A. in press (astro-ph/0310063)
Pichardo B, Vazquez-Semadeni E, Gazol A, Passot T, Ballesteros-Paredes J. 2000. On
the Effects of Projection on Morphology. ApJ. 532:353-360
Piehler G, Kegel WH 1995. The formation of interstellar molecular lines in a turbulent
velocity field with finite correlation length. A&A. 297:841-853
Piontek RA, Ostriker EC. 2003. Thermal and Magnetorotational Instability in the ISM:
Two-Dimensional Numerical Simulations. ApJ. in press (astroph/0310510)
Plume R, Jaffe DT, Evans NJ, Martin-Pintado J, Gomez-Gonzalez J. 1997. Dense gas and
star formation: Characteristics of cloud cores associated with water masers. ApJ.
476:730-749
Plume R, Bensch F, Howe J et al. 2000. Large-scale
Orion A. ApJ. 539:L133-L136
13
CO J=54 and [C I] Mapping of
Politano H, Pouquet A. 1995. Model of intermittency in magnetohydrodynamic
turbulence. Phys.Rev.E. 52:636-641
Politano H, Pouquet A, Carbone V. 1998. Determination of anomalous exponents of
structure functions in two-dimensional magnetohydrodynamic turbulence.
Europhys.Lett. 43:516-521
Pope SB. 2000. Turbulent Flows. Cambridge: Cambridge University Press, pp 771
Porter D, Woodward P, Pouquet A. 1998. Inertial range structures in decaying
compressible turbulent flows. Phys. Fluids. 10:237-245
Porter D, Pouquet A, Sytinea I, Woodward P. 1999. Turbulence in compressible flows.
Physica A . 263:263-270
Porter D, Pouquet A, Woodward P. 2002. Measures of intermittency in driven supersonic
flows. Phys. Rev. E. 66:026301-1--026301-12
Pouquet A, Frisch U, Leorat J. 1976. Strong MHD helical turbulence and the nonlinear
dynamo effect. J. Fluid Mech. 77:321-354
Pullin DI, Saffman PG. 1998. Vortex dynamics in turbulence. Ann. Rev. Fluid Mech.
30:31-51
Pumir A. 1996. Turbulence in homogeneous shear flows. Phys. Fluids. 8:3112-3127
Pushkarev A, Resio D, Zakharov V. 2003. Weak turbulent approach to the windgenerates gravity sea waves. Physica D. 184:29-63
Radjai F, Roux S. 2002. Turbulentlike Fluctuations in Quasistatic Flow of Granular
Media. Phys. Rev. Lett. 89:064302-1-064302-4
Rickett BJ. 1970. Interstellar scintillation and pulsar intensity variations. MNRAS.
150:67-91
Ricotti M, Ferrara A. 2002. What regulates the velocity distribution of interstellar clouds?
MNRAS. 334:684-692
Roberts WW. 1969. Large-Scale Shock Formation in Spiral Galaxies and its Implications
on Star Formation. ApJ . 158:123-143
Rosen A, Bregman JN, Norman ML. 1993. Hydrodynamical simulations of star-gas
interactions in the interstellar medium with an external gravitational potential. ApJ.
413:137-149
Rosolowsky EW, Goodman AA, Wilner DJ, Williams JP 1999. The Spectral Correlation
Function: A New Tool for Analyzing Spectral Line Maps. ApJ. 524:887-894
Rotman D. 1991. Shock wave effects on a turbulent flow. Phys. Fluids A. 3:1792-1806
Ryden BS. 1996. The Shapes of Dense Cores and BOK Globules. ApJ. 471:822-831
Saffman PG. 1971. On the spectrum and decay of random two-dimensional vorticity
distributions at large Reynolds number. Stud. Appl. Math. 50:377-383
Sakamoto S, Sunada K. 2003. Small-scale structure of low-density gas in a dark cloud
envelope: Kinematic evidence for phase transition? ApJ. 594:340-346
Salpeter EE. 1969. Pulsar amplitude variations. Nature. 221:31-33
Sanchez-Salcedo FJ, Vazquez-Semadeni E, Gazol A. 2002. The Nonlinear Development
of the Thermal Instability in the Atomic Interstellar Medium and Its Interaction with
Random Fluctuations. ApJ. 577:768-788
Sarson GR, Shukurov A, Nordlund A, Gudiksen B, Brandenburg A. 2003. Self-regulating
supernovae heating in interstellar medium simulations. Dordrecht:Kluwer. astroph/0307013
Sasao T. 1973 On the Generation of Density Fluctuations Due to Turbulence in SelfGravitating Media. PASJ. 25:1-33
Scalo JM. 1977. Heating of dense interstellar clouds by magnetic ion slip - A constraint
on cloud field strengths. ApJ. 213:705-711
Scalo JM. 1984. Turbulent velocity structure in interstellar clouds. ApJ. 277:556-561
Scalo JM. 1987. Theoretical approaches to interstellar turbulence. In Interstellar
Processes. ed. DJ Hollenbach, HA Thronson Jr. pp. 349-392. Dordrecht:Reidel.
Scalo J. 1990. Perception of interstellar structure - Facing complexity. In Physical
processes in fragmentation and star formation. ed. R Capuzzo-Dolcetta, C Chiosi, A
DiFazio. pp. 151-176. Dordrecht: Kluwer.
Scalo J, Vazquez-Semadeni E, Chappell D, Passot T. 1998. On the Probability Density
Function of Galactic Gas. I. Numerical Simulations and the Significance of the Polytropic
Index. ApJ. 504:835-853
Schekochihin AA, Maron JL, Cowley SC, McWilliams JC. 2002. The Small-Scale
Structure of Magnetohydrodynamic Turbulence with Large Magnetic Prandtl Numbers.
ApJ. 576:806-813
Scheffler H. 1967. Interstellare absorption III. Zur wolkenstruktur des interstellaren
staubes. Zeit. fur Ap. 65:60-83
Schlichting H, Gersten K. 2000. Boundary Layer Theory, 8th ed. Berlin: Springer. Chap.
16.5.4. pp. 799
Schlegel DJ, Finkbeiner DP, Davis M. 1998. Maps of Dust Infrared Emission for Use in
Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds.
ApJ. 500:525-553
Schneider S, Elmegreen BG. 1979. A catalog of dark globular filaments. ApJS. 41:8795
Sellwood JA, Balbus SA. 1999. Differential Rotation and Turbulence in Extended H I
Disks. ApJ . 511:660-665
Semelin B, de Vega HJ, Sanchez N, Combes F. 1999. Renormalization group flow and
fragmentation in the self-gravitating thermal gas. Phys. Rev. D. 59:125021-40
Seto N. Yokoyama J. 1998. Sample Variance of the Cosmic Velocity Field. ApJ.
496:L59-L62
She Z -S. 1991. Intermittency and non-gaussian statistics in turbulence. Fluid Dyn. Res.
8:1
She Z-S, Chen S, Doolen G, Kraichnan RH, Orszag SA 1993. Reynolds number
dependence of isotropic Navier-Stokes turbulence. Phys. Rev. Lett. 70:3251-3254
She Z-S, Leveque E. 1994. Universal scaling laws in fully developed turbulence.
Phys.Rev.Lett. 72:336-339
Shebalin JV, Matthaeus WH, Montgomery D. 1983. Anisotropy in MHD turbulence due
to a mean magnetic field. J. Plasma Phys. 29:525-547
Shivamoggi BK. 1997. Equilibrium statistical mechanics of compressible isotropic
turbulence. Europhys. Lett. 38:657-662
Shukurov A. Sarson GR, Nordlund A, Gudiksen B, Brandenburg A et al. 2002. The
effects of spiral arms on the multi-phase ISM. astroph/0212260
Simon R, Jackson JM, Clemens DP, Bania TM, Heyer MH. 2001. The structure of four
molecular cloud complexes in the BU-FCRAO Milky Way galactic ring survey. ApJ.
551:747-763
Smith MD, Mac Low M-M, Zuev JM. 2000a. The shock waves in decaying supersonic
turbulence. A&A. 356:287-300
Smith JM, Mac Low M-M, Heitsch F. 2000b. The distribution of shock waves in driven
supersonic turbulence. A&A. 362:333-341
Snyder PB, Hammett GW, Dorland W. 1997. Landau fluid models of collisionless
magnetohydrodynamics. Phys. Plasmas. 4:3974-3985
Solomon PM, Rivolo AR, Barrett J, Yahil A. 1987. Mass, luminosity, and line width
relations of Galactic molecular clouds. ApJ. 319:730-741
Spitzer L Jr. 1968. Diffuse Matter in Space. New York: Interscience. pp. 170
Sreenivasan KR. 1991. Fractals and Multifractals in Fluid Turbulence. Ann.Rev.Fluid
Mech. 23:539-604
Sreenivasan KR, Antonia RA. 1997. The phenomenology of small-scale turbulence.
Ann. Rev. Fluid Mech. 29:435-472
Sreenivasan KR, Dhruva B. 1998. Is there scaling in high-Reynolds-number turbulence?
Prog. Theor. Phys. Suppl. 130:103-120
Stanimirovic S, Staveley-Smith L, Dickey JM, Sault RJ, Snowden SL. 1999. The largescale HI structure of the Small Magellanic Cloud. MNRAS. 302:417-436
Stanimirovic S, Staveley-Smith L, van der Hulst JM, Bontekoe TJR, Kester DJM, Jones
PA. 2000. Cool dust and gas in the Small Magellanic Cloud. MNRAS. 315:791-807
Stanimirovic S, Lazarian A. 2001. Velocity and Density Spectra of the Small Magellanic
Cloud. ApJ. 551:L53-L56
Stenholm LG. 1984. The fluctuation spectrum of molecular clouds. A&A. 137:133-137
Stone JM, Ostriker EC, Gammie CF. 1998. Dissipation in Compressible
Magnetohydrodynamic Turbulence. ApJ. 508:L99-L102
Stutzki J, Bensch F, Heithausen A, Ossenkopf V, Zielinsky M. 1998. On the fractal
structure of molecular clouds. A&A. 336:697-720
Tabeling P. 2002. Two-dimensional turbulence: a physicist approach. Phys.Rep. 362:162
Tabeling P, Willaime H. 2002. Transition at dissipative scales in large-Reynolds-number
turbulence. Phys. Rev. E. 65:066301-1--066301-5
Tachihara K, Onishi T, Mizuno A, Fukui Y. 2002. Statistical study of C18O dense cloud
cores and star formation. A&A. 385:909-920
Tagger M, Falgarone E, Shukurov A. 1995. Ambipolar filamentation of turbulent
magnetic fields. A&A. 299:940-946
Takaoka M. 1995. Non-Gaussian probability distribution of a velocity field in uniform
straining-flow turbulence. Phys. Rev E. 52:3827-3834
Tauber JA, Goldsmith PF, Dickman RL 1991. The smoothness of CO line profiles in
Orion - Implications for clumpiness. ApJ. 375:635-641.
Tennekes H, Lumley JL. 1972. A first course in turbulence. Cambridge, MA. MIT Press.
300 pp.
Thomasson M, Donner KJ, Elmegreen BG. 1991. Simulations of the effect of spiral arms
on the cloud-ensemble velocity dispersion. A&A . 250:316-323
Troland TH, Heiles C. 1986. Interstellar magnetic field strengths and gas densities
Observational and theoretical perspectives. ApJ. 301:339-345
Truelove JK, Klein RI, McKee CF, Holliman JH II, Howell LH, Greenough JA. 1997.
The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of
Isothermal Self-gravitational Hydrodynamics. ApJ. 489:L179-L183
Tsinober A. 2001. An Informal Introduction to Turbulence. Dordrecht: Kluwer. 324 pp.
Tsytovich VN. 1972. An introduction to the theory of plasma turbulence. Oxford:
Pergamon Press. vii. 135 pp.
Vainshtein SI. 2003. Most singular vortex structures in fully developed turbulence.
arXiv:physics/0310008
van Buren D. 1985. The initial mass function and global rates of mass, momentum, and
energy input to the interstellar medium via stellar winds. ApJ . 294:567-577
Vazquez-Semadeni E. 1994. Hierarchical Structure in Nearly Pressureless Flows as a
Consequence of Self-similar Statistics. ApJ. 423:681-692
Vazquez-Semadeni E. 1999. Turbulence in molecular clouds. In Millimeter-Wave
Astronomy: Molecular Chemistry & Physics in Space, ed. WF Wall, A Carraminana, L
Carrasco. pp. 171-194. NY: Kluwer Academic.
Vazquez-Semadeni E, Passot T, Pouquet A. 1995. A turbulent model for the interstellar
medium. 1: Threshold star formation and self-gravity. ApJ. 441:702-725
Vazquez-Semadeni E, Gazol A. 1995. Gravitational instability in a turbulent, nonuniform media. A&A 303:204-210
Vazquez-Semadeni E, Passot T, Pouquet A. 1996. Influence of Cooling-induced
Compressibility on the Structure of Turbulent Flows and Gravitational Collapse. ApJ.
473:881-893
Vazquez-Semadeni E, Ballesteros-Paredes J, Rodriguez LF. 1997. A Search for LarsonType Relations in Numerical Simulations of the ISM: Evidence for Nonconstant Column
Densities. ApJ. 474:292-307
Vazquez-Semadeni E, Canto J, Lizano S. 1998. Does turbulent pressure behave as a
logatrope? ApJ. 492:596-602
Vazquez-Semadeni E, Ostriker EC, Passot T, Gammie CF, Stone JM. 2000.
Compressible MHD Turbulence: Implications for Molecular Cloud and Star Formation.
In Protostars and Planets IV. ed. V Mannings, AP Boss, SS Russell. pp. 3-28.
Tucson:Univ. of Ariz.
Vazquez-Semadeni E, Gazol A, Scalo J. 2000. Is Thermal Instability Significant in
Turbulent Galactic Gas? ApJ. 540:271-285
Vazquez-Semadeni E, Garcia N. 2001. The Probability Distribution Function of Column
Density in Molecular Clouds. ApJ. 557:727-735
Vestuto JG, Ostriker EC, Stone, JM. 2003. Spectral Properties of Compressible
Magnetohydrodynamic Turbulence from Numerical Simulations. ApJ. 590:858-873
Vishniac ET. 1994. Nonlinear instabilities in shock-bounded slabs. ApJ . 428:186-208
Vogelaar MGR, Wakker BP. 1994. Measuring the fractal structure of interstellar clouds,
A&A. 291:557-568
Vollmer B, Beckert T. 2002. Turbulent viscosity in clumpy accretion disks. Application
to the Galaxy. A&A . 382:872-887
Vollmer B, Beckert T. 2003. Turbulent viscosity in clumpy accretion disks. II. Supernova
driven turbulence in the Galaxy. A&A . 404:21-34
von Hoerner S. 1951. Eine Methode zur Untersuchung der Turbulenz der interstellaren
Materie. Mit 10 Textabbildungen. Zeit.Astrop. 30:17-64
von Weizsacker CF. 1951. The Evolution of Galaxies and Stars. ApJ. 114:165-186
Wada K, Norman CA. 1999. The Global Structure and Evolution of a Self-Gravitating
Multiphase Interstellar Medium in a Galactic Disk. ApJ. 516:L13-L16
Wada K, Spaans M, Kim S. 2000. Formation of Cavities, Filaments, and Clumps by the
Nonlinear Development of Thermal and Gravitational Instabilities in the Interstellar
Medium under Stellar Feedback. ApJ. 540:797-807
Wada K, Norman CA. 2001. Numerical Models of the Multiphase Interstellar Matter
with Stellar Energy Feedback on a Galactic Scale. ApJ. 547:172-186
Wada K, Meurer G, Norman CA. 2002. Gravity-driven Turbulence in Galactic Disks.
ApJ. 577:197-205
Wakker BP 1990. Interstellar neutral hydrogen at high velocities. PhD Dissertation Rijks
Universiteit Groningen. 179pp.
Walder R. Folini D. 1998. Knots, filaments, and turbulence in radiative shocks. A&A .
330:L21-L24
Waleffe F. 1992. The nature of triad interactions in homogeneous turbulence. Phys.
Fluids A. 4:350-363
Wentzel DG. 1968a. Hydromagnetic Waves Excited by Slowly Streaming Cosmic Rays.
ApJ. 152:987-996
Wentzel DG. 1969b. Pulsar Scintillations due to Distant Streaming Cosmic Rays. ApJ.
156:L91-L95
Westpfahl DJ, Coleman PH, Alexander J, Tongue T. 1999. AJ. The Geometry of the H I
of Several Members of the M81 Group: The H I Is Fractal. AJ. 117:868-880
Wilson OC, Minich G, Flather E, Coffeen MF. 1959. Internal Kinematics of the Orion
Nebula. ApJS. 4:199-256
Wilson RW, Jefferts KB, Penzias AA. 1970. Carbon Monoxide in the Orion Nebula.
ApJ. 161:L43-L44
Xie T. 1997. On Scaling Laws and Alfvenic Magnetic Fluctuations in Molecular Clouds.
ApJ. 475:L139-L142
Xu J, Stone JM. 1995. The Hydrodynamics of Shock-Cloud Interactions in Three
Dimensions. ApJ . 454:172-181
Yeung PK, Brasseur JG. 1991. The response of isotropic turbulence to isotropic and
anisotropic forcing at the large scales. Phys.Fluids. 3:884-897
Yue ZY, Zhang R, Winnewisser G, Stutzki J. 1993. On the clumpy structure of molecular
clouds. Ann. Phys. 2:9-25
Zakharov V, L'vov V, Falkovich G. 1992. Kolmogorov Spectra of Turbulence.
Berlin:Springer. 254 pp.
Zank GP, Matthaeus WH. 1993. Nearly incompressible fluids. II:
Magnetohydrodynamics, turbulence, and waves. Phys. of Fluids A. 5:257-273
Zhang X, Lee Y, Bolatto A, Stark AA. 2001. CO (J=4-->3) and [C I] Observations of the
Carina Molecular Cloud Complex. ApJ. 553:274-287
Zhou Y. 1993. Degrees of locality of energy transfer in the inertial range. Phys. Fluids
A. 5:1092-1094
Zhou Y, Yeung PK, Brasseur JG 1996. Scale disparity and spectral transfer in anisotropic
numerical turbulence. Phys. Rev. E. 53:1261-1264
Zielinsky M, Stutzki J. 1999. The relation of the Allan- and Delta- variance to the
continuous wavelet transform. A&A. 347:630-633
Zuckerman B, Palmer P. 1974. Radio radiation from interstellar molecules. ARAA.
12:279-313
Zuckerman B, Evans NJ II. 1974. Models of massive molecular clouds. ApJ. 192:L149L152
Zweibel EG. 2002. Ambipolar Drift in a Turbulent Medium. ApJ. 567:962-970
Zweibel EG, McKee, CF. 1995. Equipartition of energy for turbulent astrophysical fluids:
Accounting for the unseen energy in molecular clouds. ApJ. 439:779-792
Zweibel EG, Brandenburg A. 1997. Current Sheet Formation in the Interstellar Medium.
ApJ. 478:563-568