|Observation data (J2000 epoch)|
|Right ascension||14h 11m 20.6s|
|Declination||+52° 12′ 21″|
|Distance||4.6 billion light-years
(Light travel time)
5.6 billion light-years
|Apparent magnitude (V)||19.8|
|Apparent size (V)||2 Mly diameter|
|DA 360, 3C 295, 4C 52.30, QSO B1409+524|
3C 295 is a narrow-line radio galaxy located in the constellation of Boötes. With a redshift of 0.464, it is approximately 5 billion light-years from Earth. At time of the discovery of its redshift in 1960, this was the remotest object known.
The radio galaxy itself is a fairly normal small radio galaxy although unusually its hotspots are readily detected in optical and X-ray emission. The X-ray emission from the source is dominated by thermal emission from a rich cluster of galaxies. In optical images about 100 galaxies can be seen. 3C 295's cluster has enough material to create another 1,000 galaxies or more, making it one of the most massive objects in the known Universe. However, X-ray data showed that there is not enough mass to hold 3C 295 together gravitationally, which suggests the presence of dark matter.
- "NASA/IPAC Extragalactic Database". Results for 3C 295. Retrieved 2007-04-19.
- "3C 295". XJET: X-Ray Emission from Extragalactic Radio Jets. 2004-07-16. Retrieved 2010-04-06.
- Daniel Stern & Hyron Spinrad. "Search Techniques for Distant Galaxies (Table 1)". as represented in the NASA/IPAC Extragalactic Database Level 5 (A Knowledgebase for Extragalactic Astronomy and Cosmology), curated by Cren Frayer. Bibcode:1999PASP..111.1475S. Retrieved 2010-04-29.
- Hardcastle, M.J. "An optical inverse-Compton hotspot in 3C196?". Archived from the original on 2007-09-30. Retrieved 2007-04-20.
- Nemiroff, R.; Bonnell, J., eds. (25 November 1999). "3C 295: X-rays From A Giant Galaxy". Astronomy Picture of the Day. NASA. Retrieved 2007-04-20.
- www.jb.man.ac.uk/atlas/ (J. P. Leahy)