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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2609
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dc.contributor.authorCowsik, R-
dc.contributor.authorFriedlander, Michael. W-
dc.date.accessioned2008-07-09T09:17:41Z-
dc.date.available2008-07-09T09:17:41Z-
dc.date.issued1995-05-
dc.identifier.citationAstrophysical Journal, Part 2 - Letters, Vol. 444, No. 1, pp. L29 - L32en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/2609-
dc.description.abstractThe 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.extent709349 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995ApJ...444L..29Cen
dc.subjectCosmic Raysen
dc.subjectGamma Ray Spectraen
dc.subjectHydrogenen
dc.subjectInterstellar Gasen
dc.subjectLine Spectraen
dc.subjectOrion Nebulaen
dc.subjectEnergy Budgetsen
dc.subjectIonizationen
dc.subjectRadiant Flux Densityen
dc.subjectSpectrum Analysisen
dc.titleThe implications of gamma-ray lines observed from the Orion complexen
dc.typeArticleen
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