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The H.E.S.S. Galactic Plane Survey

Published online by Cambridge University Press:  21 October 2010

Emma de Oña-Wilhelmi
Emma de Oña-Wilhelmi*
Affiliation:
Max-Planck-Institute für Kernphysik, P.O. Box 103980, D 69029 Heidelberg, Germany email: [email protected]
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Abstract

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The H.E.S.S. Galactic Plane Survey (GPS) has revealed a large number of Galactic Sources, including Pulsar Wind Nebulae (PWN), Supernova Remnants (SNRs), giant molecular clouds, star formation regions and compact binary systems, as well as a number of unidentified objects, or dark sources, for which no obvious counterparts at other wavelengths have yet been found. We will review the latest results from the GPS observations and discuss the most interesting cases.

Keywords

gamma rays: observations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 808
Copyright
Copyright © International Astronomical Union 2010

References

Aharonian, F. A. et al. (H. E. S. S. Collaboration) 2005, Science, 307, 1938.CrossRefGoogle Scholar
Aharonian, F. A. et al. (H. E. S. S. Collaboration) 2006, ApJ, 636, 777.CrossRefGoogle Scholar
Aharonian, F. A. et al. (H. E. S. S. Collaboration), 2008, A&A, 477, 353.Google Scholar