Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1416
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dc.contributor.authorBhat, C. L-
dc.date.accessioned2007-03-14T06:25:36Z-
dc.date.available2007-03-14T06:25:36Z-
dc.date.issued1990-
dc.identifier.citationBASI, Vol. 18, pp. 215-227en
dc.identifier.urihttp://hdl.handle.net/2248/1416-
dc.description.abstractExperimental evidence is reported for the discovery of an entirely new class of gamma-ray binary objects involving a magnetic white dwarf rather than a neutron star degenerate primary. These sources may have photon energies extending into the PeV range. The gamma-ray light curves exhibit a striking morphological similarity with corresponding phase dependence of the circularly polarized light from the sources. If confirmed, these results will have important consequences for the physics underlying acceleration of high-energy particle beams in binary systems as well as for the contribution of unresolved point sources in the Galactic gamma-ray backgrounden
dc.format.extent441455 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectPolarsen
dc.subjectBinariesen
dc.titleGamma ray observations of polarsen
dc.typeArticleen
Appears in Collections:BASI Publications

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