Gamma-ray emissions from pulsar binaries
The launch of the Fermi Gamma-ray Space Telescope marked a new era in observing gamma-rays from astrophysical sources. Fermi’s high sensitivity in the ~ 0.1−300GeV energy range opens an important window in the observation of the gamma-ray emissions from pulsar binaries, which emit most of their radi...
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| Language: | English |
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The University of Hong Kong (Pokfulam, Hong Kong)
2014
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| Online Access: | http://hdl.handle.net/10722/206456 |