Leo Cluster
Leo Cluster | |
---|---|
Observation data (Epoch J2000) | |
Constellation(s) | Leo |
Right ascension | 11h 44m 29.5s[1] |
Declination | 19° 50′ 21″[1] |
Brightest member | NGC 3842 |
Number of galaxies | ~100[2] |
Richness class | 2[3] |
Bautz-Morgan classification | II-III[3] |
Redshift | 0.022 (6 595 km/s)[1] |
Distance (co-moving) |
97.8 Mpc (319.0 Mly) h−1 0.705 |
X-ray flux | (81.40 ± 6.0%)×10−12 erg s−1 cm−2 (0.1—2.4 keV)[1] |
Other designations | |
Abell 1367 | |
See also: Galaxy groups, Galaxy clusters, List of galaxy clusters | |
The Leo Cluster (Abell 1367) is a galaxy cluster about 330 million light-years distant (z = 0.022[1]) in the constellation Leo. Along with the Coma Cluster, it is one of the two major clusters comprising the Coma Supercluster.
See also
References
- 1 2 3 4 5 "NASA/IPAC Extragalactic Database". Results for Abell 1367. Retrieved 2007-10-04.
- ↑ "Abell 1367". Albert Highe: Observing Projects. Retrieved 2007-10-04.
- 1 2 Abell, George O.; Corwin, Harold G., Jr.; Olowin, Ronald P. (May 1989). "A catalog of rich clusters of galaxies" (PDF). Astrophysical Journal Supplement Series 70 (May 1989): 1–138. Bibcode:1989ApJS...70....1A. doi:10.1086/191333. ISSN 0067-0049. Retrieved March 12, 2012.
External links
- The Coma Supercluster with images of A1367
- Leo-Galaxienhaufen (Abell 1367)
- Abell 1367 - The Leo Galaxy Cluster
Coordinates: 11h 44m 29.5s, +19° 50′ 21″
|
|
This article is issued from Wikipedia - version of the Monday, February 22, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.