"Galaxy groups" refers to a collection of galaxies that are close together and interact with one another. It is a smaller scale than galaxy clusters but bigger than individual galaxies.
Full definition
Small galaxy groups are about 1000 times more common than large clusters, so there should be many more Bullet - like groups.
The difficulty of studying the movements of dwarf satellites around their hosts varies according to the
target galaxy group.
This is a list
of galaxy groups within 100 million light years according to P Fouqué and co-workers.
Nearly all of the nearby galaxies lie near this plane (the supergalactic coordinate system was originally invented because many
nearby galaxy groups lie close to this plane.)
Note the absence of any major
galaxy groups above us on the map, this area is known as the Local Void, it is a sparse region of space with a diameter of over 100 million light years although it is not completely empty - there are some individual galaxies populating this region.
We present the magnification estimator and apply it to an X-ray selected sample of
galaxy groups in the COSMOS HST survey.
«
Distant galaxy group contradicts common cosmological models, simulations: Astronomers find plane of dwarf satellites orbiting Centaurus A.» ScienceDaily.
In the small
galaxy group HCG 62 (left), the gas is concentrated in the core (red).
«Rich groups of galaxies like the Coma Cluster are very, very rare, but there are quite a few galaxies the size of NGC 1600 that reside in average -
size galaxy groups,» Ma said.
A new clue comes from high - resolution radio observations of NGC 253 (shown), an edge - on spiral galaxy just 11 million light - years from Earth and the largest member of the so - called
Sculptor galaxy group.
Hubble photometry of one of the three
galaxy groups identified at z ~ 8, with the galaxies in the image labeled with their corresponding approximate photometric redshifts.
This map shows 600 of the brightest galaxies within 7.5 degrees of the centre of the cluster - this is an arbitary border, there are many other galaxies beyond this limit especially to the south of the cluster where there are several
additional galaxy groups.
The Virgo III Groups form a very obvious line of
galaxy groups on the left side of the Virgo cluster.
Another large collection of spiral galaxies in Canes Venatici, the dominant members are probably M106, NGC 4096 and NGC 4490, but there are many
other galaxy groups in this area of the sky and this whole region is known as the Canes Cloud.
Observed DLRGs are therefore more likely than random galaxies to be found
near galaxy groups and clusters.
The Leo II Groups are a large collection of
galaxy groups clustered about 30 million light years to one side of the Virgo cluster.
Most of these distances have been determined by Igor Karachentsev and his colleagues at the Special Astrophysical Observatory in Russia who specialise in studying the
neighbouring galaxy groups.
The galaxies in the two groups are physically close to each other and the groups seem to not be moving relative to each other, so they are often identified as a
single galaxy group.
[4] This work made use of the 3D map
of galaxy groups, provided by the Galaxy And Mass Assembly project (GAMA), following extensive observations on the Anglo - Australian Telescope.
Earlier this year, Jean - Paul Kneib of Caltech and his colleagues analyzed gravitational distortions produced by
a galaxy grouping named CL0024 +1654.
It is made up of at least 43
galaxy groups and clusters that contain about 400 galaxies in total, giving it a combined mass 20 million billion times that of our sun.
A diagram of all
the galaxy groups listed above plotted onto the supergalactic plane.
IC 335 is part of
a galaxy group containing three other galaxies, and located in the Fornax Galaxy Cluster 60 million light - years away.
These galaxy groups stretching away from the Virgo cluster are called the Virgo III cloud.
At least 100
galaxy groups and clusters are located within this Virgo Supercluster.