Canes II Group
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The Canes II Group or Canes Venatici II Group (CVn II Group) is a
group of galaxies A galaxy group or group of galaxies (GrG) is an aggregation of galaxies comprising about 50 or fewer gravitationally bound members, each at least as luminous as the Milky Way (about 1010 times the luminosity of the Sun); collections of galaxies ...
about 26.1 million light-years away from
Earth Earth is the third planet from the Sun and the only astronomical object known to harbor life. While large volumes of water can be found throughout the Solar System, only Earth sustains liquid surface water. About 71% of Earth's surfa ...
. The group resides in the
Local Supercluster The Virgo Supercluster (Virgo SC) or the Local Supercluster (LSC or LS) is a mass concentration of galaxies containing the Virgo Cluster and Local Group, which itself contains the Milky Way and Andromeda galaxies, as well as others. At leas ...
. G. De Vaucouleurs, 1975. ''Nearby Groups of Galaxies'', ch. 5. the nearer groups within 10 megaparsecs. Published in "Galaxies and the Universe," ed. by A. Sandage, M. Sandage and J. Kristian The largest galaxy within the cluster is M106 (NGC 4258), which is a
barred spiral galaxy A barred spiral galaxy is a spiral galaxy with a central bar-shaped structure composed of stars. Bars are found in about two thirds of all spiral galaxies, and generally affect both the motions of stars and interstellar gas within spiral galaxies ...
.


Galaxies in the Cluster

Canes II is directly behind Canes I, which makes it difficult to show which galaxy belongs in which cluster. It is generally accepted that the following galaxies belong in Canes II;


References


See also

* Canes I Group (CVn I GrG) * Canes Venatici Cloud Galaxy clusters Virgo Supercluster Canes Venatici {{galaxy-cluster-stub