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Temperature Structure in Merging Coma Cluster of Galaxies
Published online by Cambridge University Press: 25 May 2016
Extract
The Coma cluster has been recognized as an archetype of rich and relaxed clusters, until recent ROSAT observations reveal that the intracluster medium (ICM) has a complex distribution (Briel et al. 1992; White et al. 1993). The X-ray surface brightness distribution shows a secondary peak around the galaxy NGC 4839, at 40' SW from the cluster center.
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- Session 1: Plasma and Fresh Nucleosynthesis Phenomena
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- Copyright © Kluwer 1998