AY202a Galaxies & Dynamics Lecture 5: Galactic Structure Spirals NFW Calculate structure of CDM Halos Isothermal over large range of radii Shallower at the center Steeper past virial radius NFW 1997, ApJ 490, 493 “A Universal Density Profile from Heirarchical Clustering” ρ(r) ρcrit δc = (r/r ) (1 + r/r )2 s s where rs is a scale radius, δc is a characteristic density and ρcrit = 3H2/8πG is the critical density. Disk Kinematics Disk kinematics are driven by differential rotation. Generally the inner stuff has a shorter rotation period than the outer stuff. Ω(r) = v(r)/r Angular Rotation Rate ☼ GC Differential Rotation Disk Kinematics Next, what is the distribution of stellar radial velocities as a function of distance and of galactic longitude? l = longitude ☼ v☼ d d = star dist l S R☼ Solar dist vr R☼ 90+α * α = angle α R between vr and l.o.s. α Thus the observed radial velocity of the star S vS = vR cos(α) - v☼ sin(l) by law of sines sin(l) R so vS = ( sin(90+α) cos(α) = = R☼ R☼ vR R☼ R ) sin(l) - v☼ sin(l) vS = (Ω(R) - Ω☼) R☼ sin(l) and the transverse velocity is vT = (Ω(R) - Ω☼) R☼ cos(l) - Ω(R) d so 0 0 0 < l < 90 vS d 900 < l < 1800 If we look very locally, such that d << R (Ω(R) - Ω☼) ~ (dΩ/dR) (R R ) ☼ R☼ These expressions were expanded by J. Oort who introduced two constants to describe the local galactic velocity field: The local SHEER =A The local VORTICITY = B Oort’s Constants A =( -r dΩ ) 1 B = - 2r 2 = ½ ( dr R☼ v(r) - dv(r) ) r dr R☼ d v(r) dv(r) 2 dr (r Ω(r)) = - ½ [ r + dr ]R☼ with these definitions vS = A d sin(l) vT = d (Acos(2l) + B) Ω☼ = A – B (ang speed at Sun) Best Current Estimates: From Hipparcos A = 14.8 ± 0.8 km/s/kpc B = -12.4 ± 0.6 km/s/kpc Ω☼ = v/R = A-B = 27.2 km/s/kpc independently we think v☼~ 220 km/s, R☼~8.2 kpc Ω☼ = 26.8 km/s/kpc Vertical Structure of the Disk Now that you’ve seen how thin/thick the disk of the MW is, how is it described? Oort derived the relation describing vertical structure, equating surface potential with kinetic energy: 1 ∂(ν v2) = - ∂Φ ν ∂z ∂z where ν = # density of stars, ρ = mass density and v 2 = velocity dispersion Adding Poisson’s Equation: ∂2Φ = 4π G ρ 2 ∂z ∂ 1 ∂(νv 2) [ ν ∂ z ] = -4 πGρ ∂z thus the derivatives of the stellar density distribution and velocity dispersion w.r.t. z provide a measure of the integrated mass density in the disk, ρ0 = ρ(R☼,z=0) = the Oort Limit Current best estimate from Hipparcos + dispersion measures ~ 0.15 ± 0.02 M☼/pc3 this is about twice the density of stars + gas + dust actually measured in the Solar neighborhood disk dark matter exists. Surface Mass Density Also, we can calculate the integrated surface mass density of the disk (same formalism): +z μ(z) = ∫ ρ(z’)dz’ = -z 1 ∂(ν v 2) 2πGν ∂z which gives μ(700pc) ~ 75 M☼/pc2 the mean surface mass-density inside 700pc Spiral Galaxy Structure What gives Spiral Galaxies their appearance? There are 2 main components (plus others less visible) Disk --- rotationally supported --- thickness is a function of the local vertical “pressure” vs gravity Spiral Pattern --- Three models Density Wave Tidal Interactions SPSF = self propagating star formation Density Waves Lin’s “Grand Design” spirals (M81, M83) Interaction Induced Spirals Good Looking spirals with Friends (M51) Self Propagating Star Formation --detonation waves, SF driven by SF, “Flocculent” Spirals M81 Classic Grand Design Spiral Another GD Spiral M51 Interacting System Optical Molecular Gas -CO M33 A Flocculent System NGC4414 another Flocculent S Spiral Structure Some Definitions: Number of Arms = m, most spirals have m=2, i.e. twofold symmetry Arm Orientation: Leading rotation Trailing Density Wave Theory Developed over many years by first Bertil Lindblad, then C.C. Lin, then Frank Shu: Quasi-stationary Spiral Structure Hypothesis (spiral pattern changes only slowly w. time) + Density Wave Hypothesis Pattern is a SF pattern driven by density change Follow the Mass Density Response of Stellar Disk Gravitational Field due to Stars & Gas + Density Response of Gaseous Disk Total material needed to maintain the field || = TOTAL RESPONSE Consider the “Pattern Speed” ΩP of a fixed pattern in a differentially rotating disk of stars which are in closed orbits. As in very early (and wrong) models of the Solar system, closed elliptical stellar orbits can be approximated by circular orbits + epicycles. The Epicyclic Frequency, κ, can be calculated from the disk rotation speed and the stellar angular momentum: ( dΩ2 ) κ2 = R dR + 4Ω2 Epicyclic Frequency 4Ω2) d(r κ2 = r-3 dr ∂2Φeff =( ) 2 ∂R Angular momentum In the rotating frame Φeff = Φ(R,z) + LZ2/2R2 term And since Ω(r) = L/r2 km/s/kpc κ2 = r + 4Ω2 = 2 Ω (1 100 50 dΩ2 dr -½ – A/B) Ω + κ/2 Ω Generally ΩP = Ω –nκ/m Ω – κ/2 5 r 10 Ω-κ The features seen in the rotation curve and overall pattern are then (1) Pattern Speed ΩP (2) Physical Rotation Ω(R) (3) Co-rotation Radius Rc, ΩP = Ω(RC) (4) Inner and Outer Lindblad Resonances corresponding to closed orbits at the pattern speed --ΩP = Ω(R) ± κ/m • A Rotation Pattern with Two Inner LB Resonances ΩP Lindblad first noted that for n=1, m=2 (Ω – κ/2) is constant over a large range of radii such that ΩP = Ω – κ/2 and that a pattern could exist and be moderately stable. C.C. Lin computed the response of stars & gas: Assume that the gravitational potential is a superposition of plane waves in the disk: Φ (r,φ,t) = -2πGμ |K| eiK(r,t)(r-r0) uniformly rotating sheet Where K = wave number = 2π/λ and μ = surface density Now find a dispersion relation if μ(r,φ,t) = H(r,t) ei(mφ + f(r,t)) then -2πG Φ(r,φ,t) = |K| H(r,t) e-i(mφ + f(r,t))