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Flattening of galaxies of different morphological types in subclusters of Coma

โœ Scribed by N. G. Kogoshvili; T. M. Borchkhadze; A. T. Kalloghlian

Publisher
Springer
Year
2007
Tongue
English
Weight
66 KB
Volume
50
Category
Article
ISSN
0571-7256

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From the structural investigations of 19 clusters of galaxies follows that sccondary maxima in their projccted radial galaxy distributions can be explained by subclustcring. There are no signs for density shells around the cluster centres. Subclustering seems to be a typical phenomenon in clusters o