DEPARTMENT OF ASTRONOMY

COURSE WEB PAGES


ASTRONOMY 386C
Properties of Galaxies
Spring 2002
    Unique No. 45655 TTH 12:30-2:00 RLM 15.216B



4. DISK GALAXIES

4.1 Surface Photometry

  • Radial brightness profiles of bulges and disks:
    • Analytic fitting functions
  • Disk parameter corrrelations
  • Bulge-disk decomposition
  • Vertical brightness pro files of disks:
    • Analytic fitting functions
  • Thick disks

4.2 Bulge Dynamics

  • Evidence that some “bulges” are really disks
  • Revised bulge-to-total luminosity ratios as function of Hubble type

4.3 Vertical Structure of Thin Disks: Theory

  • The isothermal sheet

4.4 Local Stability of Disks

  • Jeans instability: velocity dispersion stabilizes small-scale perturbations
  • Rotation stabilizes large-scale perturbations
  • Complete stability: Toomre ’s Q parameter
  • Observations: Q in the Galactic solar neighborhood
  • Observations: Q in other galaxy disks
  • Other disk heating mechanisms:
    • Lumps: the Spitzer-Schwarzschild mechanism
    • Scattering by bars and spiral structure
    • Heating by accreted satellites

4.5 Spiral Structure

  • Observations of global spiral structure
  • Epicyclic theory
  • Kinematic spiral density waves
  • Dynamical spiral density waves
  • Swing amplification
  • Observational consequences and tests
  • Alternatives:
    • Self-propagating star formation and flocculent spirals
    • Tidal spirals

4.6 Bars

  • Observed properties of SB galaxies: bars, rings, and lenses
  • Formation and evolution of bars: n-body simulations
  • Importance of bars: secular evolution
    • Orbits in barred potentials
    • Radial transport of gas; star formation
    • Stellar-dynamical secular evolution <= density redistribution, angular momentum transport
    • Formation or box-shaped bulges and lenses (?)

4.7 Kinematics of the Galactic Solar Neighborhood

  • Standards of rest
  • Effects of galactic rotation
    • Intuitive picture
    • Global formulae
    • Local approximations
  • Random velocities in the solar neighborhood: velocity ellipsoid
  • Asymmetric drift

4.8 Global Structure of the Galaxy

  • The Hubble type of the Galaxy
  • Galactic parameters
  • Thin disk (Population I)
  • Stellar halo (Population II)
  • Thick disk (Intermediate Population II)
  • Evidence that the Galaxy is barred

4.9 Warps in Galaxy Disks

  • Observations (mostly HI)
  • The problem: formation and maintenance of warps
  • The solution: triaxial dark halos?


 
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29 October 2001
UT Astronomy Program • The University of Texas at Austin • Austin, Texas 78712
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