Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.9901d&link_type=abstract
American Astronomical Society, 183rd AAS Meeting, #99.01; Bulletin of the American Astronomical Society, Vol. 25, p.1438
Astronomy and Astrophysics
Astronomy
Scientific paper
The interstellar clouds in Orion, which comprise the nearest giant molecular cloud complex, are good subjects for study of the diffuse, high energy (E > 30 MeV) gamma ray emission that results from cosmic ray interactions with the interstellar medium. The large angular size of the Orion complex and the unprecedented sensitivity and resolution of the EGRET instrument on the Compton Gamma Ray Observatory permit the search for variations in the gamma ray production function and the N(H_2)/W_CO ratio within the complex. Because of the recent and ongoing massive star formation in Orion, analysis of the gamma ray emission can be related to proposed mechanisms of cosmic ray production. We will present an analysis of the EGRET observations of the Orion complex obtained in the first two years of the operation of GRO, and a comparison with the findings from the study by Bloemen et al. (1984, A&A 139, 37) using COS-B data.
Bertsch David L.
Digel Seth William
Dingus Brenda Lynn
Esposito Joseph A.
Fichtel Carl E.
No associations
LandOfFree
High Energy Gamma Ray Emission from the Interstellar Clouds in Orion does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with High Energy Gamma Ray Emission from the Interstellar Clouds in Orion, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Energy Gamma Ray Emission from the Interstellar Clouds in Orion will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-781052