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Gamma-ray line astronomyGamma-ray astronomy is a valuable source of information on solar activity, supernovae, and nucleosynthesis. Cosmic gamma-ray lines were first observed from solar flares and more recently from the galactic center and a transient event. The latter may give an important insight into nuclear reactions taking place near neutron stars and black holes and a measure of the gravitational redshifts of such objects.
Document ID
19790043841
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ramaty, R.
(NASA Goddard Space Flight Center Laboratory for High Energy Astrophysics, Greenbelt, Md.; Washington University, St. Louis, Mo., United States)
Lingenfelter, R. E.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 9, 2013
Publication Date
March 8, 1979
Publication Information
Publication: Nature
Volume: 278
Subject Category
Astrophysics
Accession Number
79A27854
Funding Number(s)
CONTRACT_GRANT: NSF AST-78-10289
Distribution Limits
Public
Copyright
Other

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