Abell 520. Imaged January 2012.
|Observation data (Epoch J2000)|
|Right ascension||04h 54m 03.80s|
|Declination||+02° 53′ 33.00″|
|Number of galaxies||289+|
|Velocity dispersion||1,066 km/s|
|811 Mpc (2,645 Mly) h−1
|ICM temperature||9.8 keV|
|Binding mass||17×1014 h−1
|X-ray luminosity||14.44×1044 erg/s (0.1–2.4 keV)|
|X-ray flux||8.4×10−12 erg s−1 cm−2 (0.1–2.4 keV)|
|The Train Wreck Cluster|
|See also: Galaxy groups, Galaxy clusters, List of galaxy clusters|
The Abell 520 galaxy cluster is an unusual structure resulting from a major merger. It has been popularly nicknamed The Train Wreck Cluster, due to its chaotic structure, and is classified as a Bautz-Morgan type III cluster. It is at a co-moving radial distance of 811 Mpc (2,645 Mly) and subtends 25 arcminutes on the sky.
At one time, this cluster appeared to present a challenge prevailing theories about dark matter as well as most alternative theories of modified gravity, because its dark matter content appeared to be distributed in a way which was very different to the usual pattern, and which did not have a simple explanation based on dark matter that only interacts gravitationally. As a result, at one time it was believed that the distribution of the dark matter was the result of a novel mechanism associated with large scale filaments rather than galaxies. An analysis of the motions of 293 galaxies in the cluster field suggested that Abell 520 was a cluster forming at the crossing of three filaments of the large scale structure.
However, more precise observations since this time have shown that the earlier observations were misleading, and that the distribution of dark matter and its ratio to normal matter are very similar to those in galaxies in general, making novel explanations unnecessary. 
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- Universe Today, Galaxy Cluster Collision Creates a Dark Matter Core
- Dark Matter Core Defies Explanation