期刊
ASTROPARTICLE PHYSICS
卷 29, 期 1, 页码 63-69出版社
ELSEVIER
DOI: 10.1016/j.astropartphys.2007.11.008
关键词
gamma rays : theory; TeV gamma rays; TeV sources
The detection by the HESS atmospheric Cerenkov telescope of 14 new sources from the Galactic plane makes it possible to estimate the contribution of unresolved sources like those detected by HESS to the diffuse Galactic emission measured by the Milagro Collaboration. The number intensity relation and the luminosity function for the HESS source population are investigated. By evaluating the contribution of such a source population to the diffuse emission we conclude that a significant fraction of the TeV energy emission measured by the Milagro experiment could be due to unresolved sources like HESS sources. Predictions concerning the number of sources which Veritas, Milagro, and HAWC should detect are also given. (c) 2007 Elsevier B.V. All rights reserved.
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