Implications of γ-ray lines observed from the orion complex. II

dc.contributor.author	Cowsik, R
dc.contributor.author	Friedlander, W. M
dc.date.accessioned	2009-09-16T10:20:39Z
dc.date.available	2009-09-16T10:20:39Z
dc.date.issued	1995
dc.identifier.citation	Iucci, N and Lamanna, E., eds., 24th International Cosmic Ray Conference, Vol. 2, held August 28 - September 8, 1995 in Rome, Italy. pp. 253 - 255	en
dc.identifier.uri	http://hdl.handle.net/2248/4823
dc.description.abstract	The observation of intense gamma-ray line emission from the Orion complex, attributed by Bloemen et al. to de-excitation of cosmic-ray carbon and oxygen nuclei, has important, implications for emission from Orion in the infrared and in high-energy gamma rays, and also for the theories of cosmic-ray origins. Some of these implications are briefly pointed out.	en
dc.language.iso	en	en
dc.publisher	International Union of Pure and Applied Physics	en
dc.relation.ispartofseries	International Cosmic Ray Conference;Vol. 2
dc.relation.uri	http://adsabs.harvard.edu/abs/1995ICRC....2..253C	en
dc.subject	Implications of γ-Ray Lines	en
dc.subject	Intense Gamma-Ray Line Emission	en
dc.subject	Orion Complex	en
dc.subject	Cosmic-Ray Carbon	en
dc.subject	Cosmic-Ray Oxygen Nuclei	en
dc.subject	High-Energy Gamma Rays	en
dc.subject	Theories of Cosmic-Ray Origins	en
dc.title	Implications of γ-ray lines observed from the orion complex. II	en
dc.type	Article	en