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
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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