Astronomy:Abell 1795
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Short description: Galaxy cluster in the constellation of Boötes
| Abell 1795 | |
|---|---|
| Observation data (Epoch J2000) | |
| Constellation(s) | Boötes |
| Right ascension | 13h 49m 00.5s[1] |
| Declination | +26° 35′ 07″[1] |
| Richness class | 2[2] |
| Bautz–Morgan classification | I [2] |
| Redshift | 0.062476 (18 730)[1] |
| Distance (co-moving) | 266 Mpc (868 Mly) h−10.705[1] |
| ICM temperature | 6.12 keV[3] |
| Binding mass | 6.03×1014[3] M☉ |
| X-ray flux | (68.10 ± 5.8%)×10−12 erg s−1 cm−2 (0.1–2.4 keV)[1] |
Abell 1795 is a galaxy cluster in the Abell catalogue.
Black holes
In January 2014, scientists using data collected by the Chandra X-Ray Observatory and other telescopes reported they had found evidence of a new supermassive black hole candidate disrupting a star in a dwarf galaxy in the Abell 1795 cluster.[4][5]
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 "NED results for object ABELL 1795". NASA/IPAC Extragalactic Database (NED). http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=Abell+1795&extend=no.
- ↑ 2.0 2.1 Abell, George O.; Corwin, Harold G. Jr.; Olowin, Ronald P. (May 1989). "A catalog of rich clusters of galaxies". Astrophysical Journal Supplement Series 70 (May 1989): 1–138. doi:10.1086/191333. ISSN 0067-0049. Bibcode: 1989ApJS...70....1A.
- ↑ 3.0 3.1 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". The Astrophysical Journal (Chicago, Illinois, USA) 640 (2): 691–709. doi:10.1086/500288. Bibcode: 2006ApJ...640..691V.
- ↑ "Chandra Press Room :: Death By Black Hole In Small Galaxy? :: 08 January 14" (in en). http://chandra.harvard.edu/press/14_releases/press_010814.html.
- ↑ Boen, Brooke (2015-05-06). "Dwarf Galaxy, Galaxy Cluster Abell 1795" (in en). NASA. https://www.nasa.gov/mission_pages/chandra/multimedia/white-dwarf-system-abell-1795.html.
Coordinates: 
13h 49m 00.5s, +26° 35′ 07″
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