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...
| Main Authors: | , , , |
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| Format: | Journal Article |
| Published: |
EDP Sciences
2010
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| Online Access: | http://hdl.handle.net/20.500.11937/25936 |