Astronomy:Abell 1835
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Short description: Galaxy cluster in the constellation Virgo
| 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) | 3,296 Gpc (10,750 Gly) h−10.705 [1] |
| X-ray flux | (11.30 ± 7.3%)×10−11 erg s−1 cm−2 (0.1–2.4 keV)[1] |
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
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "NASA/IPAC Extragalactic Database". Results for Abell 1835. http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=ABELL+1835&img_stamp=yes&extend=no&hconst=70.5&omegam=0.27&omegav=0.73&corr_z=1.
- ↑ 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. doi:10.1086/191333. ISSN 0067-0049. Bibcode: 1989ApJS...70....1A. http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?bibcode=1989ApJS...70....1A&page_ind=0&epage_ind=137&type=PRINTER&data_type=PDF_HIGH&email=&emailsize=500&emailsplit=YES&send=GET&verified=YES. Retrieved March 12, 2012.
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″
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