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High energy survey of supernova remnants with BATSEThe burst and transient source experiment (BATSE) survey of the high energy emission from supernova remnants is reported on. The ability of BATSE to continuously monitor the entire sky in the 20 keV to 2 MeV energy range enables a large group of remnants to by studied at high energies. Preliminary analysis indicates the likely detection of several supernova remnants other than the Crab nebula. Among these are MSH 15-52, Vela, Cas A and possibly HB 9. The techniques employed are discussed together with the status of the survey and its limitations.
Document ID
19970025844
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
McCollough, M. L. (NASA Marshall Space Flight Center Huntsville, AL United States)
Wilson, C. A. (NASA Marshall Space Flight Center Huntsville, AL United States)
Zhang, S. N. (NASA Marshall Space Flight Center Huntsville, AL United States)
Harmon, B. A. (NASA Marshall Space Flight Center Huntsville, AL United States)
Date Acquired
August 17, 2013
Publication Date
March 1, 1997
Subject Category
Astronomy
Accession Number
97N25314
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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