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Leo II Groups

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(Redirected from NGC 3190 Group) Series of galaxy clusters
Leo II Groups
The Leo II Groups of galaxies
Observation data (Epoch )
Right ascension10 00 to 11 40
Declination0° to +35°
Number of galaxiesat least 110
Parent structureVirgo Supercluster
Distance65 Mly (20 Mpc) to 95 Mly (29 Mpc)
Other designations
Leo II Cloud
References:

The Leo II Groups, or Leo II Cloud, are a series of at least 110 galactic clusters and individual galaxies stretching approximately 30 Mly (9.2 Mpc) ecliptic west of the edge of the Virgo cluster. It is located approximately 65 Mly (20 Mpc) to 95 Mly (29 Mpc) from the Solar System, at a right ascension of 10 00 to 11 40 .

These clusters include:

See also

References

  1. ^ Powell, Richard (July 30, 2006). "The Virgo II Groups". An Atlas of the Universe. Archived from the original on July 22, 2012. Retrieved August 9, 2022.
  2. Powell, Richard (February 23, 2003). "The Universe within 100 million Light Years". Durham University. Archived from the original on August 8, 2022. Retrieved August 8, 2022.
  3. "NAME NGC 3166 Group". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved August 9, 2022.
  4. Makarov, Dmitry; Karachentsev, Igor (April 21, 2011). "Galaxy groups and clouds in the local (z~ 0.01) Universe". Monthly Notices of the Royal Astronomical Society. 412 (4): 2498–2520. arXiv:1011.6277. Bibcode:2011MNRAS.412.2498M. doi:10.1111/j.1365-2966.2010.18071.x. S2CID 119194025.
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