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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1930
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dc.contributor.authorBhattacharya, S-
dc.contributor.authorKaul, R. K-
dc.contributor.authorKaul, C. L-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2007-10-27T11:46:15Z-
dc.date.available2007-10-27T11:46:15Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 185 - 189en
dc.identifier.urihttp://hdl.handle.net/2248/1930-
dc.description.abstractWe estimate the integral γ-ray fluxes above 10 MeV photon energy, likely to result from neutral pion decay, following photomeson interactions between ultra-high energy protons accelerated in Supernova Remnants (SNR) and the background non-thermal X-ray photon field. Taking SN1006 as a test case, we find that the intergral fluxes in the TeV range are significantly lower than the experimentally reported values, indicating the ineffectiveness of the photo-meson interaction as a source of the reported Tev γ-ray signal from SNR.en
dc.format.extent331002 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..185Ben
dc.subjectGamma rayen
dc.subjectPhoto-mesonen
dc.subjectSupernova Remnants(SNR)en
dc.titleGamma ray production in SNR's -contribution from photomeson processen
dc.typeArticleen
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