On the origin of the Orion energetic particles

Details On the origin of the Orion energetic particles On the origin of the Orion energetic particles

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1064p&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1064-1068 (1997).

Other

Molecular Clouds, H2 Clouds, Dense Clouds, And Dark Clouds, Associations Of Stars In The Milky Way, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

We present a series of arguments leading to a model for the Orion gamma-ray emission. In particular, we address the crucial question of the origin of the energetic particles interacting with the molecular cloud complex. We show that it is very unlikely that these particles are accelerated within the clouds themselves, and propose that they originate from the Orion-Eridanus superbubble, located in front of the Orion clouds. Generalisation to other OB association-molecular cloud pairs is possible.

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