Supernova remnants interacting with molecular clouds as seen with H.E.S.S

D. Fernandez; H. Laffon; I. Oya; J. Mehault; M. Dalton; M. Renaud (for the H.E.S.S. Collaboration); P. Eger; S. Ohm

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Supernova remnants interacting with molecular clouds as seen with H.E.S.S

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arxiv 1305.6396 v1 pith:LVWN2P6T submitted 2013-05-28 astro-ph.GA astro-ph.HE

D. Fernandez , M. Dalton , P. Eger , H. Laffon , J. Mehault , S. Ohm , I. Oya , M. Renaud (for the H.E.S.S. Collaboration) This is my paper · ORCID

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keywords cloudsinteractingmolecularremnantssnrssupernovasystemsaccelerated

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About 30 Galactic supernova remnants (SNRs) are thought to be physically associated with molecular clouds (MCs). These systems are prime \g-ray source candidates as the accelerated particles from shock fronts collide with the surrounding high-density medium thus emitting gamma-rays through hadronic interactions. However only a handful of such interacting SNRs are detected at TeV energies. We report the current status of the High Energy Stereoscopic System (H.E.S.S.) observations towards these SNR-MC systems, with a particular emphasis on the latest results.

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