Probing cosmic ray acceleration through molecular clouds in the vicinity of supernova remnant with H.E.S.S.

Details Probing cosmic ray acceleration through molecular clouds in the vicinity of supernova remnant with H.E.S.S. Probing cosmic ray acceleration through molecular clouds in the vicinity of supernova remnant with H.E.S.S.

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..361f&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc

Astronomy and Astrophysics

Astronomy

2

Cosmic Rays, Molecular Clouds, H2 Clouds, Dense Clouds, And Dark Clouds, Astronomical And Space-Research Instrumentation, Supernova Remnants

Scientific paper

Several very high energy γ-ray excesses have been recently detected by H.E.S.S. towards known associations between supernova remnants and molecular clouds. Such associations are very interesting as dense molecular clouds in the vicinity of supernova blast waves could be a probe of proton acceleration. A hadronic scenario could explain part or the overall of these excesses.

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