Study of Galactic Sources with H.E.S.S.

Details Study of Galactic Sources with H.E.S.S. Study of Galactic Sources with H.E.S.S.

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphcs..60..135h&link_type=abstract

Journal of Physics: Conference Series, Volume 60, Issue 1, pp. 135-138 (2007).

Physics

Scientific paper

The H.E.S.S. imaging air Cherenkov telescope array has performed a blind survey at energies above 100 GeV of parts of the Galactic plane as well as dedicated (deeper) observations of gamma-ray source candidates. New sources including shell type super-nova remnants, pulsar-wind nebulae, binary systems, cosmic ray illuminated molecular clouds, as well as unidentified sources have been found. In this contribution, a selected overview of the recent results focussing on shell type supernova remnants and pulsar wind nebulae is given.

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