Abell 1835
| Abell 1835 | |
|---|---|
|
|
| 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
References
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<references />, or <references group="..." />External links
- Abell 1835 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Coordinates: 
14h 01m 00s, +02° 51′ 00″
| Morphology | |
|---|---|
| Structure | |
| Active nuclei | |
| Energetic galaxies | |
| Low activity | |
| Interaction | |
| Lists | |
| See also | |
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