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The distribution of atomic gas and dust in nearby galaxies – III. Radial distributions and metallicity gradients

✍ Scribed by H. C. Thomas; P. Alexander; M. S. Clemens; D. A. Green; L. Dunne; S. Eales

Book ID
110837705
Publisher
John Wiley and Sons
Year
2004
Tongue
English
Weight
672 KB
Volume
351
Category
Article
ISSN
0035-8711

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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