A review article for non-specialists, Physics Reports,
321, 1, 1999
GALAXY COLLISIONS
Curtis Struck
Dept of
Physics and Astronomy,
Iowa State
University, Ames, IA 50010 USA
E-mail:
curt@iastate.edu
Abstract. Theories of how galaxies, the fundamental constituents
of large-scale
structure, form and evolve have undergone a dramatic paradigm shift in the
last few decades. Earlier views were of rapid, early collapse and
formation of
basic structures, followed by slow evolution of the stellar populations and
steady buildup of the chemical elements. Current theories emphasize
hierarchical buildup via recurrent collisions and mergers, separated by long
periods of relaxation and secular restructuring. Thus, collisions between
galaxies are now seen as a primary process in their evolution.
This article
begins with a brief history; we then tour parts of the vast array of
collisional forms that have been discovered to date. Many examples are
provided to illustrate how detailed numerical models and multiwaveband
observations have allowed the general chronological sequence of
collisional morphologies to be deciphered, and how these forms are
produced by the processes of tidal kinematics, hypersonic gas dynamics,
collective dynamical friction and violent
relaxation.
Galaxy collisions may trigger the formation of a large
fraction of all the stars ever formed, and play a key role in fueling
active galactic nuclei. Current understanding of the processes involved
is reviewed. The last decade has seen exciting new discoveries about how
collisions are orchestrated by their environment, how collisional
processes depend on environment, and how these environments depend on
redshift or cosmological time.
Table of Contents
- 1. INTRODUCTION TO COLLIDING GALAXIES
- 1.1 Overview
- 1.2 Orders of Magnitude
- 1.3 Background and Early History
- 1.4 The Importance of Collisions
- 1.5 Nature's Galaxy Experiments
- 2. SOME PHENOMENOLOGY: WHAT'S OUT THERE?
- 2.1 Morphological Classification of
Collisional Forms
- 2.2 Physical Classification?
- 2.3 The Naming of Things
- 3. TRANSIENT EVENTS I: SOME WAVE
MORPHOLOGIES AND THEIR CAUSES (Yxx).
- 3.1 Ring galaxies (YDe0)
- 3.2 Symmetric Caustic Waves
- 3.3 Ring relatives: Bananas, Swallows
and Others
- 3.4 From Rings to Spirals
- 3.5 Tidal Spirals and Oculars
(YDx+)
- 3.6 Fan Galaxies and One Arms
(YDx-)
- 3.7 Gas vs. Stars in Waves
- 4. TRANSIENT EVENTS II: DEATH AND
TRANSFIGURATION.
- 4.1 Transient Mass Transfer and
Bridges
- 4.1.1 Splashes: Bridges and Infall
in Direct Collisions (YDd0)
- 4.1.2 Models and Splash Physics
- 4.1.3 Slings: Tidally Torqued
Bridges (YDx+)
- 4.1.4 Observations of Tidal Bridges
and Star Formation
- 4.2 Complete Collisional
Disruption
- 4.3 Transient Summary
- 5. COMING BACK (Ixx, Oxx)
- 5.1 Dynamical Friction - Bringing it
Back - Background and history - Recent Developments
- 5.2 Simulational Examples of Dynamical
Friction
- 5.2.1 Sinking satellites
- 5.2.2 Bobbing satellites
- 5.3 Halo Braking
- 5.4 Tidal Stretching: Tails and
"Antennae" (IXd+)
- 5.5 Shells and Ripples
- 5.6 Induced Bars
- 5.6.1 Collisional Bar Formation
- 5.6.2 Effects of Induced Bars
- 5.6.3 Longevity, Frequency and Other
Matters
- 5.7 Intermediate Summary
- 6. MERGERS - ALL THE WAY BACK (Oxx)
- 6.1 Overview and Historical
Highlights
- 6.2 Major Merger Dynamics
- 6.2.1 Violent Relaxation
- 6.2.2 Gas Funneling
- 6.3 Minor mergers: disk heating and
aging
- 6.4 New disks
- 6.4.1 Ellipticals with Disks
- 6.4.2 Counter-rotating Disks in
S0 and Sa Galaxies
- 6.4.3 Polar Ring Galaxies
- 6.5 Multiple Mergers
- 7. INDUCED STAR FORMATION
- 7.1 Color, Halpha; and Other
Indicators of Global Enhancements
- 7.2 Spectral Line Diagnostics
- 7.2.1 SF Histories
- 7.2.2 IMF Variations and the Example
of M82
- 7.3 SF Region Morphologies
- 7.4 Mechanisms and Modes
- 7.4.1 Star Formation
Enhancements
- 7.4.2 Star Formation
Suppression
- 8. ACTIVE GALACTIC NUCLEI IN COLLISIONAL
GALAXIES
- 8.1 Phenomenology
- 8.2 Fueling Mechanisms
- 9. ENVIRONMENTS AND REDSHIFT DEPENDENCE
- 9.1 Groups and Compact Groups
- 9.2 Dense Clusters
- 9.2.1 cD Galaxies
- 9.2.2 Collisions and Harassment in
Clusters
- 9.2.3 The Cluster Environment:
Stripping and Cluster Tidal Effects
- 9.2.4 Cluster-Cluster
Collisions
- 9.3 High-Redshift Collisions
- 10. CONCLUSIONS
- ACKNOWLEDGEMENTS
- REFERENCES