Interactions and Mergers of Galaxies
|For much of the twentieth century -- once the vast distances to galaxies was known -- galaxies were thought to be ``island universes,'' forming and evolving in isolation with no contact between one another. In this picture, the processes which shape the galaxies we see today are uniquely determined by the initial conditions under which galaxies form and processes completely internal to the galaxies themselves.|
|Figure 1: NGC 2997, a nearby spiral galaxy (Dave Malin/AAO).|
As galaxy catalogs began to grow, however, more and more examples of paired galaxies were found, as well as many peculiar galaxies with long, luminous "plumes" and "tails" emanating from their bodies. These galaxies were found to have anomalously blue colors, arguing that their star forming properties were quite different from normal galaxies. Examples were found of galaxy pairs so strongly perturbed that they were suggested as possible examples of actual merging encounters. Meanwhile, astronomers began to use computer simulation to study the effects of nearby companions on galaxies, and found that many of the properties of these peculiar galaxies could be explained through gravitational interactions and mergers of galaxies.
|From these studies, an alternative picture of galaxy evolution began to grow. Rather than evolving in isolation, galaxies are found in clusters and groups, and can interact quite strongly with their nearby companions. These interactions can have a profound impact on the properties of galaxies, resulting in intense bursts of star formation, the onset of quasar-like activity in galactic nuclei, and perhaps even the complete transformation of spiral galaxies into ellipticals. Studies of galaxies in the early Universe show a significant fraction of interacting and merging systems, and theories of cosmological structure formation indicate that most galaxies have had some form of strong interaction during their lifetime. Rather than being rare events, galaxy interactions may be the dominant process shaping the evolution of the galaxy population in general.|
| Figure 2: The Mice (NGC 4676), an interacting pair of galaxies |
(John Hibbard, NRAO).