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Alternative cooling flow modelsModels where the cooling or cooled cluster gas is reheated by conduction, by galaxy motions, and by supernovae are examined. In each case, it is difficult or impossible to reproduce the observed temperature gradient while also reducing the net rate at which cooled gas is produced. None of the models examined lead to a viable alternative cooling flow scenario.
Document ID
19890040159
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bregman, Joel N. (National Radio Astronomy Observatory Charlottesville, VA, United States)
David, L. P. (Virginia, University Charlottesville, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Subject Category
Astrophysics
Meeting Information
Meeting: NATO Advanced Research Workshop
Location: Cambridge
Start Date: June 22, 1987
End Date: June 26, 1987
Sponsors: NATO
Accession Number
89A27530
Funding Number(s)
CONTRACT_GRANT: NAGW-764
Distribution Limits
Public
Copyright
Other

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