Gamma ray emission from interstellar clouds - A plasma physical process capable of enhancing electron fluxes

Details Gamma ray emission from interstellar clouds - A plasma physical process capable of enhancing electron fluxes Gamma ray emission from interstellar clouds - A plasma physical process capable of enhancing electron fluxes

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.198..583m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 198, Feb. 1982, p. 583-588.

Physics

Plasma Physics

18

Bremsstrahlung, Cos-B Satellite, Gamma Rays, Interstellar Matter, Molecular Clouds, Relativistic Electron Beams, Astronomical Models, Flux (Rate), Nucleons, Plasma Physics, Spectrum Analysis

Scientific paper

Cos B measurements suggest that electrons play a dominant role in
gamma-ray production in the Galaxy. A process is discussed which can
significantly enhance relativistic electron intensities inside molecular
clouds. If this process is as common in the Galaxy as the theory
suggests, bremsstrahlung emission will be significantly enhanced too.

Affiliated with

Also associated with

No associations

Rating

Gamma ray emission from interstellar clouds - A plasma physical process capable of enhancing electron fluxes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Gamma ray emission from interstellar clouds - A plasma physical process capable of enhancing electron fluxes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma ray emission from interstellar clouds - A plasma physical process capable of enhancing electron fluxes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1648002