Abell 1413
| Abell 1413 | |
|---|---|
|
Abell 1413 image created from optical and near-infrared exposures taken with the Wide Field Channel of Hubble’s Advanced Camera for Surveys (ACS).[1] | |
| Observation data (Epoch J2000) | |
| Constellation(s) | Between Leo and Coma Berenices |
| Right ascension | 11h 55m 18.9s[2] |
| Declination | +23° 24′ 31″[2] |
| Richness class | 3[3] |
| Bautz-Morgan classification | I [3] |
| Redshift | 0.1427[2] |
| Distance (co-moving) |
593 Mpc (1,934 Mly) h−1 0.705 [2] |
| ICM temperature | 7.38 keV[4] |
| Binding mass | 7.57×1014[4] M☉ |
| See also: Galaxy groups, Galaxy clusters, List of galaxy clusters | |
Abell 1413 is a galaxy cluster in the Abell catalogue.
See also
References
- ↑ "Hubble reveals a super-rich galactic neighbourhood". www.spacetelescope.org. ESA/Hubble. Retrieved 11 November 2014.
- 1 2 3 4 "NED results for object ABELL 1413". NASA/IPAC Extragalactic Database (NED). Retrieved March 15, 2012.
- 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.
- 1 2 Table 4 from Vikhlinin, A.; Kravtsov, A.; Forman, W.; Jones, C.; Markevitch, M.; Murray, S. S.; Van Speybroeck, L. (April 2006). "Chandra Sample of Nearby Relaxed Galaxy Clusters: Mass, Gas Fraction, and Mass-Temperature Relation" (PDF). The Astrophysical Journal. Chicago, Illinois, USA: University of Chicago Press. 640 (2): 691–709. arXiv:astro-ph/0507092
. Bibcode:2006ApJ...640..691V. doi:10.1086/500288. Retrieved March 12, 2012.
Coordinates: 
11h 55m 18.9s, +23° 24′ 31″
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