A Constraint on Prompt Supernova Cosmic-Ray Production from Gamma-Ray Observations

Details A Constraint on Prompt Supernova Cosmic-Ray Production from Gamma-Ray Observations A Constraint on Prompt Supernova Cosmic-Ray Production from Gamma-Ray Observations

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197..369m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 197, P. 369, 1981

Astronomy and Astrophysics

Astronomy

13

Scientific paper

The consequences of prompt cosmic ray production intrinsic to supernovae are examined for supernova explosions occurring in dense molecular clouds. For reasonable parameters it is shown that prompt cosmic ray production cannot exceed 1048 erg per supernova. This suggests that cosmic ray production takes place mainly in the intercloud medium.

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