3C 295

3C 295 is a narrow-line radio galaxy located in the constellation of Boötes. With a redshift of approximately 0.46, it is approximately from Earth. At time of the discovery of its redshift in 1960, this was the List of galaxies#Most [distant galaxies|most remote object known].

History

The number in its name corresponds with it being the 295th object in the Third Cambridge Catalogue of Radio Sources. This is also where the prefix Cambridge Catalogue of Radio Sources|3C] came from.
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.