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Secondary maxima in the radial galaxy distribution of clusters of galaxies and subclustering

โœ Scribed by F. W. Baier

Publisher
John Wiley and Sons
Year
1983
Tongue
English
Weight
627 KB
Volume
304
Category
Article
ISSN
0004-6337

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โœฆ Synopsis

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 of galaxies.

Ails Strnkturiintcrsucliungcn an I 9 Galaxienhanfen folgt, clan Ncbcnmasima i n ihrcn projizicrten radialen Gnlaxicn.rrtcilungcn durch Unterstrukturen crkliirt werden kiinncn. Es gibt kcinc hiizcichcn fiir 1)ichteschalcn um die Haufenzcntren. tlntcrstrukturcn scheincn frir Galaxienhaufen typisch zu sein.

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