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
Density and Radial Velocity Strucutre of the Hydra I Cluster of Galaxies
β Scribed by F. W. Baier; H. Oleak
- Publisher
- John Wiley and Sons
- Year
- 1983
- Tongue
- English
- Weight
- 758 KB
- Volume
- 304
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Since 1971 the magnetic Ap star 52 Her has been investigated with respect to its magnetic field and radial velocity on the observational basis of 140 photographic Zeeman spectrograms obtained at the 2m-telescope in Tautenburg. Additionally. 47 normal spectrograms were used for the determination of t
## Abstract We present the Fundamental Plane (FP) of earlyβtype galaxies in the clusters of galaxies RXJ1415.1+3612 at __z__ = 1.013. This is the first detailed FP investigation of cluster earlyβtype galaxies at redshift __z__ = 1. The distant cluster galaxies follow a steeper FP relation compared
## Abstract The dynamic behavior of the concentration profiles of a single protein in the pore solution and the adsorbed phase is studied in different adsorbent media when the spatial density distribution of the immobilized ligands is either uniform or nonβuniform and at the same time the single pr