𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Investigation of Galaxy Distribution in the Ursa Major Supercluster of Galaxies

✍ Scribed by F. W. Baier


Publisher
John Wiley and Sons
Year
1980
Tongue
English
Weight
709 KB
Volume
301
Category
Article
ISSN
0004-6337

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


The distribution of galaxies in the fiel
✍ F. W. Baier; W. Mai πŸ“‚ Article πŸ“… 1978 πŸ› John Wiley and Sons 🌐 English βš– 397 KB πŸ‘ 3 views

## Abstract The number‐density distribution of four ABELL‐clusters in the region of the Hercules supercluster was derived by counting galaxies on the red Palomar Sky Survey prints. For one isolated cluster the radial number‐density distribution and the radial cumulative galaxy distribution were cal

Investigation of Galaxy Distribution in
✍ F. W. Baier πŸ“‚ Article πŸ“… 1979 πŸ› John Wiley and Sons 🌐 English βš– 793 KB

Investigation of Galaxy Distribution in 10 Clusters 1;. W. BAIER, Potsdam-Babelsberg Zentralinstitut fur Astropliysik der Akademie der Wissenscliaften der DDli With 16 figures (Keceived 1979 April 12) The number density distributions for further 10 clusters of galaxies werc derivcd by counting gala

Secondary maxima in the radial galaxy di
✍ F. W. Baier πŸ“‚ Article πŸ“… 1983 πŸ› John Wiley and Sons 🌐 English βš– 627 KB

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

Investigations of clusters of galaxies.
✍ F.W. Baier; K. Fritze; H. Tiersch; R. Ziener πŸ“‚ Article πŸ“… 1991 πŸ› John Wiley and Sons 🌐 English βš– 1008 KB

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