Astrophysics (Index)About

galaxy merger

(combination of galaxies upon collision)

The term galaxy merger is used to designate the act of two or more galaxies becoming one when colliding. Stars generally do not collide, but gas and dust clouds are affected. Such a merger is an example of a galaxy interaction, which also includes the effect of one galaxy on another just from being near enough to affect the other's gravitational field. Such close encounters can modify the shape of a galaxy, and even pull some portions of the galaxy away, e.g., tidal arms. Mergers are thought to boost star formation, specifically when gas and dust from the galaxies collide. Simulations suggest the increase in star formation rate is greatest when the galaxies have similar mass, i.e., a galaxy merger mass ratio close to 1. It is thought that mergers can trigger an active galactic nucleus (AGN).

Sometimes galaxy collisions can be clearly seen or seen to be inevitable. Merging or partial merging can be seen in trails of stars between the collided galaxies. Galactic asymmetry is a sign of a possible recent merger. A galaxy with nuclei is often a sign of a merger. Evidence of past mergers is observed in nearby galaxies, leading to the idea that mergers are common in galaxy growth. Elliptical galaxies are theorized to be a product of mergers, to the point where orderly concentric orbits have been randomized.

The galaxy merger timescale is the timescale of the duration of the merging process.

One classification of galaxy mergers is major (two galaxies of similar size, e.g., spiral galaxies, which might form an elliptical galaxy) versus minor (a small galaxy joining a large galaxy). Mergers may also be classified as local, e.g., using a cutoff at a redshift of 0.1.

The term peculiar galaxy includes apparent galaxy mergers in progress, galaxies strongly affected by lesser interactions (disturbed galaxies), and other sources of oddness, such as some AGNs.

(galaxies,mergers,collision,star formation,elliptical)
Further reading:

Referenced by pages:
Atlas of Peculiar Galaxies (APG)
black hole binary (BHB)
de Vaucouleurs' profile
dynamical friction
faint blue galaxy (FBG)
final parsec problem
galactic tide
galaxy formation
giant elliptical galaxy
gravitational wave (GW)
irregular galaxy
morphology-density relation
peculiar galaxy (p)
quenched galaxy
random forest
retrograde accretion
ring galaxy
supermassive black hole (SMBH)
tidal arm
tidal tail
Toomre sequence
ultraluminous infrared galaxy (ULIRG)