Abell 262
| Abell 262 | |
|---|---|
 | |
| Observation data (Epoch J2000) | |
| Constellation(s) | Between Andromeda and Triangulum |
| Right ascension | 01h 52m 50.4s[1] |
| Declination | +36° 08′ 46″[1] |
| Richness class | 0[2] |
| Bautz–Morgan classification | III[2] |
| Redshift | 0.0163 (4 887 km/s)[1] |
| Distance | 65.6 Mpc (214 Mly) h−1 0.705[1] |
| ICM temperature | 2.08 keV[3] |
| X-ray flux | (48.6 ± 9.9%)×10−12 erg s−1 cm−2 (0.1—2.4 keV)[1] |
Abell 262 is a galaxy cluster in the Abell catalogue.
See also
References
- ^ a b c d e "NED results for object ABELL 0262". NASA/IPAC Extragalactic Database (NED). Retrieved March 15, 2012.
{{cite web}}: CS1 maint: postscript (link) - ^ a b 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.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ^ 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. 640 (2). Chicago, Illinois, USA: University of Chicago Press: 691–709. arXiv:astro-ph/0507092. Bibcode:2006ApJ...640..691V. doi:10.1086/500288. Retrieved March 12, 2012.
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