What do supernova remnants interacting with molecular clouds reveal?

Details What do supernova remnants interacting with molecular clouds reveal? What do supernova remnants interacting with molecular clouds reveal?

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1112...54f&link_type=abstract

SCIENCE WITH THE NEW GENERATION OF HIGH ENERGY GAMMA-RAY EXPERIMENTS: Proceedings of the 6th Edition: Bridging the Gap Between G

Physics

10

Molecular Clouds, H2 Clouds, Dense Clouds, And Dark Clouds, Gamma-Ray, Supernova Remnants

Scientific paper

Very high energy γ-ray emission has been recently detected by H.E.S.S. from the direction of associations between supernova remnants and molecular clouds. In such associations dense molecular clouds may reveal accelerated cosmic rays in the vicinity of supernova remnant forward shocks. Hadronic interactions could explain part or all of the observed γ-ray fluxes. The discovery of a new VHE γ-ray source, HESS J1923+141, coincident with the supernova remnant W51C, is reported. Amongst possible associations for this source is a shocked molecular cloud.

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