High-Latitude Molecular Clouds as gamma-ray Sources for GLAST
arXiv:astro-ph/0501385 · doi:10.1086/428903
Abstract
For about two decades, a population of relative small and nearby molecular clouds has been known to exist at high Galactic latitudes. Lying more than 10 from the Galactic plane, these clouds have typical distances of 150 pc, angular sizes of , and masses of order tens of solar masses. These objects are passive sources of high-energy -rays through cosmic ray-gas interactions. Using a new wide-angle CO survey of the northern sky, we show that typical high-latitude clouds are not bright enough in -rays to have been detected by EGRET, but that of order 100 of them will be detectable by the Large Area Telescope (LAT) on GLAST. Thus, we predict a new steady population of -ray sources at high Galactic latitudes, perhaps the most numerous after active galactic nuclei.
Accepted for publication in the Astrophysical Journal Letters
References in corpus (4)
- A Uniform CO Survey of the Molecular Clouds in Orion and Monoceros
- Theoretical modelling of the diffuse emission of gamma-rays from extreme regions of star formation: The case of Arp 220
- Blazar Counterparts for 3EG Sources at -40 < decl. < 0: Pushing South Through the Bulge
- Luminous infrared galaxies as plausible gamma-ray sources for GLAST and IACTs
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- On the potential of the Cherenkov Telescope Array for the study of cosmic-ray diffusion in molecular clouds
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