Abell 2667 | |
---|---|
Observation data (Epoch J2000) | |
Constellation(s) | Sculptor |
Right ascension | 23h 51m 42s[1] |
Declination | −26° 00′ 00″[1] |
Richness class | 3[2] |
Bautz–Morgan classification | I [2] |
Redshift | 0.23000[3] |
Distance | 927 Mpc (3,023 Mly) h−1 0.705[3] |
Abell 2667 is a galaxy cluster. It is one of the most luminous galaxy clusters in the X-ray waveband known at a redshift about 0.2.
This cluster is also a well-known gravitational lens.
On 2 March 2007, a team of astronomers reported the detection of the Comet Galaxy in this cluster. [4] This galaxy is being ripped apart by the cluster's gravitational field and harsh environment. The finding sheds light on the mysterious process by which gas-rich spiral-shaped galaxies might evolve into gas-poor irregular- or elliptical-shaped galaxies over billions of years.
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