Cosmic Cannibalism
One of the most important ways that galaxies evolve is through interaction with other galaxies.
We see substantial evidence for collisions between smaller
galaxies triggering
the formation of massive luminous stars. In some cases, galaxies appear to be swallowing other
galaxies whole.
Caught in the Act
The
adjacent image taken using the 1 m European Southern Observatory telescope,
illustrates an extreme example of this. This false color image is of a distant cluster of
galaxies called Abel 3827, which lies at a redshift of 0.1, corresponding to a distance of about 1.5 billion
light years. In the enhanced image we see that the dominant central galaxy of the cluster
(the bright central region) has swallowed five other galaxies in the cluster (the five large yellow blobs
inside the central region).
In many other clusters of galaxies one
finds a large galaxy near the center, suggesting that galactic cannibalism in clusters may be relatively
common.
Cannibalism in the Early Universe?
The following figure shows a Very Large Telescope image of the distant
galaxy 1138-262 and
its vicinity.
This galaxy, which is a strong source of radio waves,
is in the southern constellation Hydra (the Water Snake), at a distance of about
10 billion light years from Earth. The light in this image left the galaxy when the Universe was only
about 20 percent of its present age.
The false color image
image is of Lyman-alpha hydrogen emission, and marks regions having a high concentration of ionized
hydrogen. The cloud of ionized hydrogen around the galaxy is about
500,000 light years across (five times the size of the visible Milky Way).
A Massive Galaxy Assembles Itself?
Observations of this galaxy by ROSAT in X-rays and the VLA
at radio frequencies suggest that it is surrounded
by a hot gas, much like that observed more locally in clusters of galaxies. Furthermore, the Hubble
Space Telescope has
found that the galaxy appears to be comprised of many clumps. The preliminary
interpretation is that this is a massive galaxy in the process of formation by
absorbing smaller galaxies in a distant rich cluster. If this is a correct interpretation, it may shed
important light on how galaxy and cluster structure grew in the early Universe.
In this interpretation, the large cloud of ionized
hydrogen gas is the material from which the smaller galaxies
that are being absorbed into the giant galaxy are
forming.