Gamma Rays from Molecular Clouds
Abstract
I discuss the spectral features of pi-0 decay gamma-radiation from clouds/targets located in proximity of relatively young proton accelerators, and speculate that such ``accelerator+target'' systems in our Galaxy can be responsible for a subset of unidentified EGRET sources. Also, I argue that the recent observations of high energy gamma-rays from the Orion complex contain evidence that the level of the ``sea'' of galactic cosmic rays may differ significantly from the flux and the spectrum of local (directly detected) particles.
Keywords
Cite
@article{arxiv.astro-ph/0012290,
title = {Gamma Rays from Molecular Clouds},
author = {F. A. Aharonian},
journal= {arXiv preprint arXiv:astro-ph/0012290},
year = {2021}
}
Comments
The paper is based on presentations at 2 meetings of the workshop on "The Astrophysics of Galactic Cosmic Rays" hosted by the International Space Science Institute, Bern, October 1999 and May 2000; to be published in Space Science Reviews