A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization

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A search for VHE counterparts of Galactic Fermi bright sources and MeV to TeV spectral characterization

Very high-energy (VHE; E > 100 GeV) γ-rays have been detected in a wide range of astronomical objects, such as pulsar wind nebulae (PWNe), supernova remnants (SNRs), giant molecular clouds, γ-ray binaries, the Galactic center, active galactic nuclei (AGN), radio galaxies, starburst galaxies, and...

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Bibliographic Details
Main Authors:	Tam, P., Wagner, S., Tibolla, Omar, Chaves, R.
Format:	Journal Article
Published:	EDP Sciences 2010
Online Access:	http://hdl.handle.net/20.500.11937/25936

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