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Studies of gas in cooling flow clustersThis report describes studies of cooling flows in rich clusters of galaxies, found to be sources of strong, extended X-ray emission seen by the EINSTEIN satellite. Two complementary lines of investigation were pursued: (1) studies of the dust content of the cluster gas using multi-wavelength data from archival records of the IUE and IRAS satellites in combination with previously obtained optical, and (2) coronal line spectroscopic studies of the bright emission systems.
Document ID
19940008486
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Hu, Esther M. (Hawaii Univ. Honolulu, HI, United States)
Cowie, Lennox L. (Hawaii Univ. Honolulu, HI, United States)
Date Acquired
September 6, 2013
Publication Date
October 31, 1991
Subject Category
Fluid Mechanics And Heat Transfer
Report/Patent Number
NAS 1.26:193597
NASA-CR-193597
Report Number: NAS 1.26:193597
Report Number: NASA-CR-193597
Accession Number
94N12959
Funding Number(s)
CONTRACT_GRANT: NAG5-1257
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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