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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2456
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dc.contributor.authorBhattacharyya, S-
dc.contributor.authorBhatt, N-
dc.contributor.authorMisra, R-
dc.contributor.authorKaul, C. L-
dc.date.accessioned2008-06-19T07:11:55Z-
dc.date.available2008-06-19T07:11:55Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 375 - 376en
dc.identifier.urihttp://hdl.handle.net/2248/2456-
dc.description.abstractWe investigate here the effect on the emitted spectrum of a black hole binary due to the presence of accelerated protons in the inner region of the accretion disk. Our study shows that e-e+ pairs and high energy -rays created in inelastic p - p collisions contribute mainly in the 1 - 10 MeV range and produce a broad feature in the spectrum in this energy range which can be verified by INTEGRAL and GLAST observations.en
dc.format.extent69305 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..375Ben
dc.subjectProtonsen
dc.subjectBlack hole binariesen
dc.titleThe Effect of Non-thermal Protons on the High Energy Spectra of Black Hole Binariesen
dc.typeArticleen
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