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Musket Ball Cluster

Musket Ball Cluster
Observation data (Epoch J2000.0[1])
Constellation(s)Cancer
Right ascension09h 16m 10.9s[1]
Declination+29° 48′ 44″[1]
Redshift0.53[2]
Other designations
Musket Ball Cluster,[3] DLSCL J0916.2+2951,[2] SHELS J0916.2+2949[1]

The Musket Ball Cluster (DLSCL J0916.2+2951) is a galaxy cluster that exhibits separation between its baryonic matter and dark matter components. The cluster is a recent merger of two galaxy clusters. It is named after the Bullet Cluster, as it is a slower collision, and older than the Bullet Cluster. This cluster is further along the process of merger than the Bullet Cluster,[3] being some 500 million years older, at 700 million years old.[4] The cluster was discovered in 2011 by the Deep Lens Survey.[2] As of 2012, it is one of the few galaxy clusters to show separation between its dark matter and baryonic matter components.[5]

  1. ^ a b c d "NAME Musket Ball Cluster". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 27 July 2014.
  2. ^ a b c Dawson, William A.; Wittman, David; Jee, M. James; Gee, Perry; Hughes, John P.; Tyson, J. Anthony; et al. (19 October 2011). "Discovery of a Dissociative Galaxy Cluster Merger with Large Physical Separation". The Astrophysical Journal Letters. 747 (2) (published March 2012): 6. arXiv:1110.4391. Bibcode:2012ApJ...747L..42D. doi:10.1088/2041-8205/747/2/L42. S2CID 119244278. L42.
  3. ^ a b Chandra X-Ray Observatory (12 April 2012). "DLSCL J0916.2+2951: Discovery of the Musket Ball Cluster". Harvard University.
  4. ^ Mark Brown (13 April 2012). "The Musket Ball Cluster is 500 million years older than the Bullet Cluster". Wired. Archived from the original on 4 March 2015. Retrieved 5 September 2017.
  5. ^ Dawson, Will (6 May 2012). "Constraining Dark Matter with the Musket Ball Cluster". Will Dawson - Cosmology Research. Archived from the original on 22 January 2015.

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