Abell 1835

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Abell 1835
Abell 1835 Hubble.jpg
Abell 1835 by Hubble Space Telescope, 3.18′ view
Credit: NASA/STScI/WikiSky
Observation data (Epoch J2000)
Constellation(s) Virgo
Right ascension 14h 01m[1]
Declination +02° 51′[1]
Richness class 0[2]
Redshift 0.25320[1]
Distance
(co-moving)
1,023 Mpc (3,337 Mly) h−1
0.705
[1]
X-ray flux (11.30 ± 7.3%)×10−11 erg s-1 cm-2 (0.1—2.4 keV)[1]
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′.[1]

In 2004, one of the galaxies lensed by this cluster was proposed to be the most distant galaxy known, Galaxy Abell 1835 IR1916.

See also[edit]

References[edit]

  1. ^ a b c d e f "NASA/IPAC Extragalactic Database". Results for Abell 1835. Retrieved 2006-11-28. 
  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[edit]

Coordinates: Sky map 14h 01m 00s, +02° 51′ 00″