Journal
ASTROPHYSICAL JOURNAL
Volume 590, Issue 1, Pages L9-L12Publisher
IOP PUBLISHING LTD
DOI: 10.1086/376670
Keywords
galaxies : clusters : individual (A1656); galaxies : evolution; galaxies : interactions; galaxies : statistics; X-rays : galaxies : clusters
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This study on the Coma Cluster suggests that there are deviations from a completely random galaxy orientation on small scales. Since we found a significant coincidence of hot-gas features identified in the latest X-ray observations of Coma with these local anisotropies, they may indicate regions of recent mutual interaction of member galaxies within subclusters that are currently falling in on the main cluster.
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