NGC 3640 Group
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NGC 3640 Group
The Leo II Groups, or Leo II Cloud, are a series of at least 110 galactic clusters and individual galaxy, galaxies stretching approximately 30 Mly (9.2 Mpc) off the right edge of the Virgo Supercluster. It is located approximately 65 Mly (20 Mpc) to 95 Mly (29 Mpc) from the Solar System, at a right ascension of to . These clusters include: *NGC 3166 Group **AGC 208443 **AGC 208444 **AGC 208457 **AGC 208535 **AGC 208537 **NGC 3156 **NGC 3165 **NGC 3166 **NGC 3169 *NGC 3190 Group **NGC 3162 **NGC 3177 **NGC 3185 **NGC 3187 **NGC 3190 **NGC 3193 **UGC 5574 *NGC 3227 Group **NGC 3213 **NGC 3226 **NGC 3227 **UGC 5675 *NGC 3254 Group **NGC 3245A **NGC 3245 **NGC 3254 **NGC 3265 **NGC 3277 *NGC 3338 Group **NGC 3338 **NGC 3346 **NGC 3389 **UGC 5832 *NGC 3370 Group **NGC 3370 **NGC 3443 **NGC 3447 **NGC 3447A **NGC 3454 **NGC 3455 **NGC 3457 **UGC 5945 *NGC 3396 Group **IC 2604 **NGC 3381 **NGC 3395 **NGC 3396 **NGC 3424 **NGC 3430 **NGC 3442 *NGC 3504 Group **NGC 3380 **NGC 3400 **NGC 34 ...
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Virgo 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 least 100 galaxy groups and clusters are located within its diameter of 33 megaparsecs (110 million light-years). The Virgo SC is one of about 10 million superclusters in the observable universe and is in the Pisces–Cetus Supercluster Complex, a galaxy filament. A 2014 study indicates that the Virgo Supercluster is only a lobe of an even greater supercluster, Laniakea, a larger, competing referent of the term Local Supercluster centered on the Great Attractor. Background Beginning with the first large sample of nebulae published by William and John Herschel in 1863, it was known that there is a marked excess of nebular fields in the constellation Virgo (near the north galactic pole). In the 1950s, French–American astronomer Gérard de Vau ...
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