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Further investigations of clusters of galaxies

✍ Scribed by F. W. Baier; W. Mai


Publisher
John Wiley and Sons
Year
1977
Tongue
English
Weight
596 KB
Volume
298
Category
Article
ISSN
0004-6337

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✦ Synopsis


Abstract

The number‐density distribution in ten clusters of galaxies was derived by counting galaxies on the red Palomar Sky Survey prints. For seven isolated clusters the radial number‐density distribution and the radial cumulative galaxy distribution were calculated.


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The number-density distributions of further g clusters of galaxies were derived by counting galaxies on the red Palomar Sky Survey prints. For all the clusters the radial number density distribution and the radial cumulative galaxy distribution were calculated. Die Anzahl-Dichte-Verteilung wurde ft

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The structure of the centre of the galaxy cluster A 1795 and its surroundings, representing different cluster components, has been investigated in several wavelength ranges. A preferred orientation deviating about 10 -20" from the north-south direction has been found for all cluster components. The