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Formation of the 255-keV annihilation line near the magnetic poles of pulsars

โœ Scribed by V. M. Kontorovich; A. B. Flanchik


Book ID
110138979
Publisher
SP MAIK Nauka/Interperiodica
Year
2004
Tongue
English
Weight
52 KB
Volume
79
Category
Article
ISSN
0021-3640

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I review our current understanding of positron sources in the Galaxy, on the basis of the reported properties of the observed 511 keV annihilation line. It is argued here that most of the disk positrons propagate away from the disk (due to the low density environment) and the resulting low surface b