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Positron-electron annihilation radiation from the Galactic CenterEvidence and arguments are presented supporting the theory that the 0.511 MeV line observed from the Galactic Center stems from photon-photon pair production near a black hole with a mass not greater than approximately 500 solar masses. Observations are reviewed and the subsequent implications on the annihilation site and the positron source are discussed. Because of the variations and line width of the e(+) - e(-) annihilation radiation from the Galactic Center, positrons must essentially be produced by a single source and annihilate in an ambient gas of density greater than 10 to the 5th/cu cm, an ionization fraction greater than 10 percent, a temperature less than 5 x 10 to the 4th K, and be confined to a region of size less than 10 to the 18th cm. Such conditions may exist in warm clouds and other IR sources within the central parsec of the Galaxy.
Document ID
19840046160
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ramaty, R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lingenfelter, R. E.
(California, University La Jolla, CA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1983
Subject Category
Astrophysics
Accession Number
84A28947
Funding Number(s)
CONTRACT_GRANT: NSG-7541
Distribution Limits
Public
Copyright
Other

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