Published October 15, 1987
| Version v1
Journal article
The alignment of galaxy clusters
Description
The large-scale alignment of galaxy clusters found by a previous author was tested on the basis of the complete sample of clusters which belong to the Bahcall and Soneira superclusters using various determinations of the clusters' position angle. For small separations, clusters do tend to point toward their neighbours, but the effect is weak. Correlation of anisotropy with cluster separation is also weak. Comparison of the observational data with theoretical models shows that for small separations the alignment is similar to the predicted in the adiabatic scenario, while for greater distances between clusters to that in the isothermal one. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 228
- Journal Issue
- 4
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 941-948
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 19015441
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ADIABATIC PROCESSES; ALIGNMENT; ANISOTROPY; CORRELATIONS; GALAXY CLUSTERS; ISOTHERMAL PROCESSES; MATHEMATICAL MODELS