Phoenix Cluster
| Phoenix Cluster | |
|---|---|
| Observation data (Epoch J2000.0) | |
| Constellation(s) | Phoenix |
| Right ascension | 23h 44m 40.9s |
| Declination | −42° 41′ 54″ |
| Redshift | 0.597 |
| Distance (co-moving) |
5.7 billion light years |
| Binding mass | 1.26–2.5×1015 M☉ |
| Other designations | |
| Phoenix Cluster, SPT-CL J 2344 -4243, SPT-CL J2344-4243 | |
The Phoenix Cluster (SPT-CL J2344-4243) is a massive, type I galaxy cluster located at its namesake constellation, the southern constellation of Phoenix.
It is one of the most massive galaxy clusters known, with the mass on the order of 2×1015M☉. Another cluster, El Gordo, also in the Phoenix Constellation, is slightly more massive. Most of the mass of the Phoenix Cluster is in the form of dark matter and its intracluster medium.
The central elliptical cD galaxy of this cluster is undergoing a massive starburst, the highest recorded in a middle of a galaxy cluster, although other galaxies at higher redshifts have a higher starburst rate (see Baby Boom Galaxy). Observations by a variety of telescopes including the GALEX and Herschel space telescopes shows that it has been converting material to stars at an exceptionally high rate of 740 M☉ per year. This is considerably higher than that of NGC 1275 A, the central galaxy of the Perseus Cluster, where stars are formed at a rate around 20 times lower, or the one per year rate of star formation in the Milky Way.
The vast stellar halo of the Phoenix Cluster central galaxy extends to over 1.1 million light years from the center, making it one of the largest galaxies known. It is 22 times the diameter of our galaxy, and its starburst activity suggests that the galaxy is still growing larger.
Phoenix Cluster is also producing more X-rays than any other known massive cluster. The central galaxy in the cluster contains vast amounts of hot gas. More normal matter is present there than the total of all the other galaxies in the cluster. Data from observations indicate that hot gas is cooling in the central regions at a rate of 3,820 solar masses per year, the highest ever recorded.
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