- Abstract:
- We present an analysis of the redshift-space power spectrum, $P(k)$, of rich clusters of galaxies based on an automated cluster catalogue selected from the APM Galaxy Survey. We find that $P(k)$ can be approximated by a power law, $P(k)\proptok^{n}$, with $n\approx-1.6$ over the wavenumber range $0.04\hr
- Publication status:
- Published
- Publisher copy:
- 10.1046/j.1365-8711.1998.01441.x
-
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 296
- Issue:
- 4
- Pages:
- 995-1003
- Publication date:
- 1997-08-28
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:676d3696-e11c-4d77-bfe0-4b7ff282c4fb
- Source identifiers:
-
45841
- Local pid:
- pubs:45841
- Language:
- English
- Keywords:
- Copyright date:
- 1997
- Notes:
-
9 pages, 7 ps figures, two style files, submitted to MNRAS. Un-xxx-ed
version available at
http://www-astro.physics.ox.ac.uk/research/preprints/aug97/cluspaper.ps.gz
Journal article
The Power Spectrum of Rich Clusters of Galaxies on Large Spatial Scales
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