Secondary maxima in the radial galaxy di
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F. W. Baier
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Article
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1983
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John Wiley and Sons
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English
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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