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
Positron production and annihilation in the Milky Way
β Scribed by Nikos Prantzos
- Publisher
- Elsevier Science
- Year
- 2006
- Tongue
- English
- Weight
- 197 KB
- Volume
- 50
- Category
- Article
- ISSN
- 1387-6473
No coin nor oath required. For personal study only.
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