Astronomy 626 Reading

Spring 2005 Joshua Barnes Wed, Fri 2:00 to 3:15

Introduction

BT 1 INTRODUCTION
1.1 An Overview of the Observations
1 Stars
2 The Galaxy
3 Other galaxies
4 Open and globular clusters
5 Groups and clusters of galaxies
6 Galactic nuclei
SG 1.1 The stars
1.2 Our Milky Way
1.3 Other Galaxies
BM 1 GALAXIES: AN OVERVIEW
1.1 Introduction
1.2 A Brief History of Galactic Astronomy
1.2.1 Photometric models of the Milky Way
1.2.2 The nature of the spiral nebulae
1.2.3 Kinematic models of the Milky Way
1.2.4 Stellar populations
1.2.5 More recent developments

Morphology & environment

BM 4.1 Morphological Classification of Galaxies
4.1.1 The Hubble sequence
4.1.2 Effects of environment
4.1.3 The galaxy luminosity function
4.1.4 The Local Group

Elliptical galaxies. I

BM 4.2 Surface Photometry of Galaxies
4.2.1 The night sky
4.2.2 Effect of seeing
4.2.3 Deprojecting galaxy images
4.3 Photometry of Elliptical Galaxies
4.3.1 Radial surface-brightness profiles of elliptical galaxies
4.3.2 Color and line-strength gradients of elliptical galaxies
4.3.3 Shapes of elliptical galaxies
4.3.4 Correlations among global parameters of elliptical galaxies
SG 6.1 Photometry
6.1.1 The shapes of elliptical galaxies
6.1.2 Twisty, disky, or boxy?

Elliptical galaxies. II

BM 8.3 The ISM in Elliptical Galaxies
8.3.1 X-ray emitting plasma
8.3.2 Cool gas in ellipticals
11.1 Measuring the Kinematics of External Galaxies
11.1.1 Mean velocities and velocity dispersions
11.1.2 Analysis of line profiles
11.1.3 Position-velocity diagrams and data cubes
11.2 The Stellar Kinematics of Elliptical Galaxies
11.2.1 Large-scale properties
11.2.2 Core properties
SG 6.2.1 Measuring stellar velocities
6.2.2 The Faber-Jackson relation and the fundamental plane
6.3 Stellar Populations and Gas
6.5.1 Rich clusters of galaxies

Disk galaxies. I

BT 6.1 1 Observations
BM 4.4 Photometry of Disk Galaxies
4.4.1 Photometric effects of dust
4.4.2 Overall shapes of disk galaxies
4.4.3 Bulge-disk decomposition
4.4.4 Shapes of bulges
4.4.5 Color and metalicity gradients in disk galaxies
4.4.6 Spiral structure in disk galaxies
4.4.7 Barred galaxies
SG 5.1.2 Surface photometry of disk galaxies
5.2.2 Cool gas in the disk
5.4.1 Observed spiral patterns
5.4.3 Barred disks
5.5 Bulges and the Centers of Disk Galaxies

Disk galaxies. II

BM 8.2 The ISM in Disk Galaxies
8.2.1 Global measures
8.2.2 Radial density profiles
8.2.3 Azimuthal distributions
8.2.4 Velocity fields of disks
8.2.5 S0 galaxies
8.2.6 Metallicities of disk galaxies
8.2.7 Magnetic fields
8.2.8 Star formation in disk galaxies
11.3 The Stellar Kinematics of Disk Galaxies
11.3.1 Bulge kinematics
11.3.2 Disk kinematics
SG 5.3 Gas Motions and the Masses of Disk Galaxies
5.3.1 The rotation curve
5.3.3 The Tully-Fisher relations
Interlude: the sequence of disk galaxies
5.6.1 Gas in groups of galaxies

Distances

BM 7.3 Relative Distance Indicators
7.3.1 Luminosities of variable stars
7.3.2 Luminosity functions
7.3.3 Novae and supernovae
7.3.4 Distances from galaxy kinematics
7.3.5 Surface brightness fluctuations
7.4 Results
7.4.1 Distances within the Local Group
7.4.2 Distances beyond the Local Group
7.4.3 The asymptotic Hubble constant

Gravitational fields

BT 2 1 General results
2.1 Spherical Systems
1 Newton's theorems
2 Potentials of some simple systems
2.2 Potential-Density Pairs for Flattened Systems
1 Plummer-Kuzmin models
2 Logarithmic potentials
2.6 3 Disk potentials via Bessel functions
SG 3.1

Orbits, integrals, & chaos

BT 3.1 Orbits in Static Spherical Potentials
1 Constants and integrals of the motion
3.2 Orbits in Axisymmetric Potentials
1 Motion in the meridional plane
2 Surfaces of section
3.3 Orbits in Planar Non-Axisymmetric Potentials
1 Two-dimensional nonrotating potential
3.4 Orbits in Three-Dimensional Triaxial Potentials
1 Nonrotating potential
SG 3.1 Motion Under Gravity
6.2.4 Stellar orbits in a triaxial galaxy

Collisionless Boltzmann equation

BT 4 1 The relaxation time
4.1 The Collisionless Boltzmann Equation
SG 3.2 Why the Galaxy isn't Bumpy: Two-Body Relaxation
3.2.1 Strong close encounters
3.2.2 Distant weak encounters
3.4 The Collisionless Boltzmann Equation

N-body methods

BT 2.8 Numerical Methods

Dark matter in disk galaxies

BT 10.1 6 Rotation curves of galaxies
7(a) Tidal radii
7(b) Disk stability
SG 5.3.2 Dark matter in disk galaxies

Shapes of elliptical galaxies

BT 4.3 The Virial Equations
SG 6.2.3 How fast should an elliptical galaxy rotate?

Dark matter in elliptical galaxies

BT 4.2 The Jeans Equations
1(d) Velocity dispersions in spherical systems
10.1 7(c) X-ray halos of elliptical galaxies
SG 6.4 Dark matter and black holes
6.4.1 Dark halos

Evidence for nuclear black holes

SG 6.4.2 Central black holes?

Local stability of disk galaxies

BT 6.2 Wave Mechanics of Differentially Rotating Disks
1 Preliminaries
3 Local stability of differentially rotating disks

Theories of spiral structure

BT 3.2 3 Nearly circular orbits: epicycles and the velocity ellipsoid
6.3 2(a) The swing amplifier
6.4 Theories of Spiral Structure
1 The Lin-Shu hypothesis
2 Other density-wave theories
3 Other theories
4 Summary

The bar instability

BT 3.3 2 Two-dimensional rotating potential
3.3 3 Weak bars
6.3 Global Stability of Differentially Rotating Disks
1 Numerical work on disk stability
2(b) Feedback loops
2(c) Physical interpretation of the bar instability
6.5 Bars
1 Bars as stellar systems
Gas dynamics in barred galaxies
Summary

Warped disk galaxies

BT 6.6 Warps

Groups, clusters & LSS

SG 7.1

Interactions & dynamical friction

BT 7.1

Mergers & starburst galaxies

BT 7.4

Spectrophotometric evolution

BT 9.1

Chemical evolution

BT 9.2

Evolution of star clusters

Processes in galactic nuclei

Populations & components of the MW

BM 10.1
10.2
10.4
10.5

Kinematics of the disk

BM 10.3

Moving groups & other relics


Dark matter in disk galaxies SG 5.3; BT 10.1.6, 10.1.7(a), 10.1.7(b)
Shapes of elliptical galaxies BT 4.3; SG 6.2.3
Dark matter in elliptical galaxies BT 10.1.7(c); SG 6.4.1
Evidence for nuclear black holes SG 6.4.2
Local stability of disk galaxies BT 6.2
Theories of spiral structure BT 6.3, 6.4
The bar instability BT 6.5
Warped disk galaxies BT 6.6
Groups, clusters & LSS SG 7.1 (to p. 289)
Interactions & dynamical friction BT 7.1
Mergers & starburst galaxies BT 7.4
Spectrophotometric evolution BT 9.1
Chemical evolution BT 9.2
Evolution of star clusters
Processes in galactic nuclei
Populations & components BM 10.1, 10.2, 10.4, 10.5
Kinematics of the disk BM 10.3
Moving groups & other relics

Joshua E. Barnes (barnes@ifa.hawaii.edu)
Last modified: December 29, 2004
http://www.ifa.hawaii.edu/~barnes/ast626_05/reading.html