The implications of gamma-ray lines observed from the Orion complex

dc.contributor.author	Cowsik, R
dc.contributor.author	Friedlander, Michael. W
dc.date.accessioned	2008-07-09T09:17:41Z
dc.date.available	2008-07-09T09:17:41Z
dc.date.issued	1995-05
dc.identifier.citation	Astrophysical Journal, Part 2 - Letters, Vol. 444, No. 1, pp. L29 - L32	en
dc.identifier.issn	0004-637X
dc.identifier.uri	http://hdl.handle.net/2248/2609
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.format.extent	709349 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	The American Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1995ApJ...444L..29C	en
dc.subject	Cosmic Rays	en
dc.subject	Gamma Ray Spectra	en
dc.subject	Hydrogen	en
dc.subject	Interstellar Gas	en
dc.subject	Line Spectra	en
dc.subject	Orion Nebula	en
dc.subject	Energy Budgets	en
dc.subject	Ionization	en
dc.subject	Radiant Flux Density	en
dc.subject	Spectrum Analysis	en
dc.title	The implications of gamma-ray lines observed from the Orion complex	en
dc.type	Article	en