Gamma Rays From Molecular Clouds View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2001-10

AUTHORS

F.A. Aharonian

ABSTRACT

High energy γ-rays from individual giant molecular clouds contain unique information about the hidden sites of acceleration of galactic cosmic rays, and provide a feasible method for study of propagation of cosmic rays in the galactic disk on scales ≤100 pc. I discuss the spectral features of π0-decay γ-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 γ-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. More... »

PAGES

187-196

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1023/a:1013845015364

DOI

http://dx.doi.org/10.1023/a:1013845015364

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1010344592


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