Galaxy formation theory - Andrew J. Benson
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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.BACKGROUND MATERIAL
- 2.1.Background Cosmology
- 2.2.Structure Formation
- 2.3.Halo Formation
- 2.3.1.Halo Mass Distribution
- 2.3.2.Halo Formation
Distribution
- 2.4.Halo Structure
- 3.PRE-GALACTIC EVOLUTION OF BARYONS
- 3.1.Cold or Hot Accretion
(Shocks)
- 3.2.Cooling
- 3.2.1.Atomic
- 3.2.2.Compton Cooling
- 3.2.3.Molecular Hydrogen
Cooling
- 3.3.Heating
- 3.3.1.Photoheating
- 3.3.2.Heating from Feedback
- 3.3.3.Preheating
- 3.3.4.Thermal Conduction
- 3.4.Fate of Cooling Gas
- 4.GALAXY INTERACTIONS
- 4.1.Galaxy Orbits
- 4.2.Gravitational Interactions
- 4.2.1.Mergers
- 4.2.2.Tidal Destruction
- 4.2.3.Harassment
- 4.3.Hydrodynamical Interactions
- 4.3.1.Ram pressure
- 5.GALACTIC STRUCTURE
- 5.1.Disk Formation
- 5.1.1.Sizes
- 5.1.2.Stability
- 5.1.3.Bars/Spiral Arms
5.2.Spheroid Formation
5.2.1.Major Mergers
5.2.2.Secular Evolution
5.2.3.Sizes
6.STAR FORMATION, AGN AND FEEDBACK
6.1.Star Formation
6.2.Black Hole Formation
6.3.Feedback
6.3.1.Supernovae/Stellar Winds
6.3.2.AGN
6.4.Chemical Enrichment
6.5.Stellar Populations
6.5.1.Steller Population
Synthesis
6.5.2.Dust Absorption and
Re-emission
6.6.Absorption by the
Intergalactic Medium
7.COMPUTATIONAL TECHNIQUES
7.1.N-body/Hydro
7.2.Semi-Analytic
7.3.Halo Occupation Distributions
8.TOPICS OF CURRENT INTEREST
8.1.The First Galaxies
8.2.The Formation and Sizes of
Galaxy Disks
8.3.The Overcooling Problem
8.4.Local Group Dwarf Satellites
8.5.The Origins of the Hubble
Sequence
9.FUTURE DIRECTIONS
10.SUMMARY
REFERENCES