|Observation data (Epoch J2000)|
|Right ascension||14h 01m|
|1,023 Mpc (3,337 Mly) h−1
|X-ray flux||(11.30 ± 7.3%)×10−11 erg s-1 cm-2 (0.1—2.4 keV)|
|See also: Galaxy groups, Galaxy clusters, List of galaxy clusters|
Abell 1835 is a galaxy cluster in the Abell catalogue. It is a cluster that also gravitational lenses more-distant background galaxies to make them visible to astronomers. The cluster has a red shift of around 75,900 km/s and spans 12′.
In 2004, one of the galaxies lensed by this cluster was proposed to be the most distant galaxy known, Galaxy Abell 1835 IR1916.
- "NASA/IPAC Extragalactic Database". Results for Abell 1835. Retrieved 2006-11-28.
- 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.
- Abell 1835 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
|This galaxy-related article is a stub. You can help Wikipedia by expanding it.|