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- W2149778321 abstract "From the structural investigations of 19 clusters of galaxies follows that secondary maxima in their projected radial galaxy distributions can be explained by subclustering. There are no signs for density shells around the cluster centres. Subclustering seems to be a typical phenomenon in clusters of galaxies. Aus Strukturuntersuchungen an 19 Galaxienhaufen folgt, daß Nebenmaxima in ihren projizierten radialen Galaxienverteilungen durch Unterstrukturen erklärt werden können. Es gibt keine Anzeichen für Dichteschalen um die Haufenzentren. Unterstrukturen scheinen für Galaxienhaufen typisch zu sein." @default.
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- W2149778321 date "1983-01-01" @default.
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- W2149778321 title "Secondary maxima in the radial galaxy distribution of clusters of galaxies and subclustering" @default.
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- W2149778321 doi "https://doi.org/10.1002/asna.2113040503" @default.
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