Abell 2667 | |
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![]() Abell 2667 from Hubble Space Telescope. Comet Galaxy is top-left (blue). | |
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 and is 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.
Abell 2667 is similar to many other low-redshift and cool-core galaxy clusters in terms of the cooling processes that happen at its center, which consists of a brightest cluster galaxy (BCG) and a supermassive black hole (SMBH). [5]
Abell 2667 acts as an intense gravitational telescope, lensing red-shifted galaxies behind it. [6] Although the warped galaxies may appear to be part of this galaxy cluster, they are in fact significantly more distant. [7]
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