Published October 1, 1984
| Published
Journal Article
Open
Relations between spatial correlations of rich clusters of galaxies
- Creators
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Politzer, H. David
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Wise, Mark B.
Abstract
The authors express the N-point rich cluster correlation function in terms of the two-point rich cluster correlation function in a model where rich clusters formed wherever suitably averaged primordial energy density fluctuations are unusually large. The validity of the results is not restricted to regions where the connected (reduced) N-point correlation functions are small compared with unity.
Additional Information
© 1984 American Astronomical Society. Provided by the NASA Astrophysics Data System. Received 1984 April 30; accepted 1984 June 22. We thank C. Hogan for many useful discussions. Work supported in part by the U.S. Department of Energy under contract DE-AC03-81-ER40050.Attached Files
Published - 1984ApJ___285L___1P.pdf
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Additional details
- Eprint ID
- 70889
- Resolver ID
- CaltechAUTHORS:20161005-151454504
- DE-AC03-81-ER40050
- Department of Energy (DOE)
- Created
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2016-10-05Created from EPrint's datestamp field
- Updated
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2019-10-03Created from EPrint's last_modified field