Abstract
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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