Leo II Groups
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) off the right edge of the Virgo Supercluster.[1][2] It is located approximately 65 Mly (20 Mpc) to 95 Mly (29 Mpc) from the Solar System, at a right ascension of 10h 00m to 11h 40m .[1]
Leo II Groups | |
---|---|
Observation data (Epoch ) | |
Right ascension | 10h 00m to 11h 40m |
Declination | 0° to +35° |
Number of galaxies | at least 110 |
Parent structure | Virgo Supercluster |
Distance | 65 Mly (20 Mpc) to 95 Mly (29 Mpc) |
Other designations | |
Leo II Cloud | |
References: [1] | |
- NGC 3166 Group
- NGC 3190 Group
- NGC 3227 Group
- NGC 3254 Group
- NGC 3338 Group
- NGC 3338
- NGC 3346
- NGC 3389
- UGC 5832
- NGC 3370 Group
- NGC 3396 Group
- IC 2604
- NGC 3381
- NGC 3395
- NGC 3396
- NGC 3424
- NGC 3430
- NGC 3442
- NGC 3504 Group
- NGC 3607 Group (Leo II Group)
- NGC 3640 Group
- NGC 3813 Group
- NGC 3755
- NGC 3813
- UGC 6603
- NGC 3810 Group[4]
- NGC 3773
- NGC 3810
- Additional galaxies in the group:
See also
References
- 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.
- 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.
- "NAME NGC 3166 Group". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved August 9, 2022.
- 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.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.