Astronomy:Virgo II Groups
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Short description: Series of galaxy clusters
Virgo II Groups | |
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The Virgo II Groups of galaxies | |
Observation data (Epoch ) | |
Right ascension | 12h 00m to 13h 30m |
Number of galaxies | at least 100 |
Distance (co-moving) | 55 Mly (16.86 Mpc) to 80 Mly (24.53 Mpc) |
Other designations | |
| |
References: [1] | |
The Virgo II Groups, also known as the Virgo II Cloud, Virgo Southern Extension, or the Virgo S Cloud, are a series of at least 100 galactic clusters and individual galaxies stretching approximately 30 megalight-years (9,198,041.81 parsecs) off the southern edge of the Virgo Supercluster.[1][2][3] It is located approximately 55 Mly (16.86 Mpc) to 80 Mly (24.53 Mpc) from the Solar System, at a right ascension of 12h 00m to 13h 30m.[1]
These clusters include:[1]
- M61 Group:
- NGC 4030 Group:
- NGC 4030
- UGC 6970
- UGC 7000
- NGC 4179 Group:
- NGC 4697 Group:
- NGC 4699 Group:
- NGC 4753 Group:
- NGC 4856 Group:
- MCG-2-33-82
- MCG-2-33-88
- MCG-3-33-32
- NGC 4856
- NGC 4984
- NGC 4995 Group:
- IC 4212
- NGC 4942
- NGC 4981
- NGC 4995
- NGC 5084 Group:
- Additional galaxies in the group:
See also
- M96 Group
- Leo II Groups
- Virgo III Groups
References
- ā 1.0 1.1 1.2 1.3 Powell, Richard (July 30, 2006). "The Virgo II Groups". An Atlas of the Universe. http://www.atlasoftheuniverse.com/galgrps/virii.html.
- ā Jiang, Fangzhou; van Dokkum, Pieter; Bezanson, Rachel; Franx, Marijn (April 10, 2012). "A nearby analog of zā¼2 compact quiescent galaxies with a rotating disk". The Astrophysical Journal Letters (The American Astronomical Society) 749 (L10): L10. doi:10.1088/2041-8205/749/1/L10.
- ā Powell, Richard (February 23, 2003). "The Universe within 100 million Light Years". Durham University. http://www.icc.dur.ac.uk/~tt/Lectures/Galaxies/LocalGroup/Back/virgo.html.
Original source: https://en.wikipedia.org/wiki/Virgo II Groups.
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