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Evidence for extended X-ray emission from globular clustersDeep exposures with the Einstein Observatory show evidence for diffuse X-ray emission from three globular clusters. One possible interpretation of these observations is that the interaction between a cluster wind and a hot gaseous galactic halo is being observed. The one cluster for which the proper motion has been measured is consistent with this interpretation.
Document ID
19820043850
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/183746
Authors
Hartwick, F. D. A. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Grindlay, J. E. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Cowley, A. P. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 10, 2013
Publication Date
March 1, 1982
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
82A27385
Distribution Limits
Public
Copyright
Other

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