The gamma-ray line emission of Orion

Details The gamma-ray line emission of Orion The gamma-ray line emission of Orion

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..425..465c&link_type=abstract

Tours symposium on nuclear physics III. AIP Conference Proceedings, Volume 425, pp. 465-472 (1998).

Physics

Nuclear Physics

Photoproduction Reactions, Spallation Reactions, Mass Loss And Stellar Winds

Scientific paper

Observations of gamma-ray emission lines of C and O in the Orion star forming region indicate that shock waves produced by stellar winds and exploding stars may be accelerating these nuclei. This mechanism may have a significant impact on the production of Li, Be, and B through spallation reactions. The nature of the acceleration makes strong predictions which may be tested by the upcoming INTEGRAL mission.

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