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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2100
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dc.contributor.authorApparao, K. M. V-
dc.date.accessioned2008-02-29T11:11:42Z-
dc.date.available2008-02-29T11:11:42Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 271 - 273en
dc.identifier.urihttp://hdl.handle.net/2248/2100-
dc.description.abstractThe hard x-ray flux resulting from inverse Compton scattering of photons from the Be star by the high energy electrons responsible for the radio emission, is calculated and compared with observation.en
dc.format.extent164480 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..271Aen
dc.subjectX-raysen
dc.subjectGamma raysen
dc.subjectBe staren
dc.titleHard X-rays and gamma rays from the Be star LSI +61-303en
dc.typeArticleen
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