Bullet Group
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Coordinates: 
08h 54m 46.5480s, −01° 21′ 37.262″
| Bullet Group | |
|---|---|
| Observation data (Epoch J2000.0[1]) | |
| Constellation(s) | Hydra |
| Right ascension | 08h 54m 46.5480s [1] |
| Declination | −01° 21′ 37.262″ [1] |
| Redshift | 0.351[1] |
| Binding mass | (2.4±0.6)×1014 [2] M☉ |
| Other designations | |
| Bullet Group,[3] SL2S J08544-0121[4] | |
| See also: Galaxy groups, Galaxy clusters, List of galaxy clusters | |
The Bullet Group (SL2S J08544-0121) is a newly merging group of galaxies, a merger between two galaxy groups to form a new larger one, that recently had a high speed collision between the two component groups. The group exhibits separation between its dark matter and baryonic matter components, and the galaxies occurring in two clumps, while the gas expanding into a billowing cloud encompassing all three clumps. As of 2014, it is one of the few galaxy clusters known to show separation between the dark matter and baryonic matter components. The group is named after the Bullet Cluster, a similar merging galaxy cluster, except on a smaller scale, being of groups instead of clusters.[2][3] The bimodal distribution of galaxies was found at discovery in 2008. The galaxy group is a gravitational lens and strongly lenses a more distant galaxy behind it, at z=~1.2[3][4]
Characteristics
As of 2014, the group is the smallest mass object to exhibit separation between its dark matter and baryonic matter components.[2]
The galaxy group is dominated by one elliptical galaxy, situated in one of the two concentrations, while the other node has two large bright galaxies, which do not dominate the group.[4] The group has an apparent radius of 200 arcseconds, and a virial radius of 1 megaparsec.[5]
See also
References
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| Morphology | |
|---|---|
| Structure | |
| Active nuclei | |
| Energetic galaxies | |
| Low activity | |
| Interaction | |
| Lists | |
| See also | |
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