Abell 2029 or A2029 is a large cluster of galaxies 315 megaparsecs (1,027 million light-years) away in the constellation Virgo. A2029 is a Bautz-Morgan classification type I cluster due to its large central galaxy, IC 1101. This type of galaxy is called a cD-type brightest cluster galaxy and may have grown to its large size by accreting nearby galaxies.
- ^ 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.
- ^ a b Walker, S. A.; Fabian, A. C.; Sanders, J. S.; George, M. R.; Tawara, Y. (March 2012). "X-ray observations of the galaxy cluster Abell 2029 to the virial radius" (PDF). eprint arXiv (Accepted for publication in the Monthly Notices of the Royal Astronomical Society). arXiv:1203.0486. Bibcode:2012MNRAS.422.3503W. doi:10.1111/j.1365-2966.2012.20860.x. Retrieved March 11, 2012.
- ^ a b NASA/IPAC EXTRAGALACTIC DATABASE. "NED results for object ABELL 2029". Retrieved March 11, 2012.
- ^ a b 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 (Chicago, Illinois, USA: University of Chicago Press) 640 (2): 691–709. arXiv:astro-ph/0507092. Bibcode:2006ApJ...640..691V. doi:10.1086/500288. Retrieved March 12, 2012.
- ^ Chandra X-ray Observatory, "Galaxy Clusters and Dark Energy: Chandra Opens New Line of Investigation on Dark Energy", Harvard-Smithsonian Center for Astrophysics
Coordinates: 15h 10m 56.20s, +05° 44′ 41″