Date and Time of the Query: 2019-06-24 T04:33:50 PDT
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Notes for object ABELL 2107

2 note(s) found in NED.

1. 2010A&A...511A..15L
Re:Abell 2107
Fujita et al. (2006) presented an analysis of Chandra observation of this
cluster. Since the cD galaxy has a large peculiar velocity and the ICM in the
central region has an irregular structure, these authors concluded that this
cluster is undergoing a merger.
From our results, A2107 contains the smallest substructure and has almost
symmetric X-ray contours providing no evidence of a recent merger.

2. 1997ApJ...482...41G
Re:ABELL 2107
This is a remarkably regular cluster. Oegerle & Hill (1992) found
evidence of substructures by using the test of D88. The peculiar velocity
of the cD galaxy could suggest a situation of nonperfect dynamical
equilibrium. However, with the present data, there is good agreement
between {sigma} and T.

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