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Gamma ray observations of polars

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dc.contributor.author Bhat, C. L
dc.date.accessioned 2007-03-14T06:25:36Z
dc.date.available 2007-03-14T06:25:36Z
dc.date.issued 1990
dc.identifier.citation BASI, Vol. 18, pp. 215-227 en
dc.identifier.uri http://hdl.handle.net/2248/1416
dc.description.abstract Experimental 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 background en
dc.format.extent 441455 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.subject Polars en
dc.subject Binaries en
dc.title Gamma ray observations of polars en
dc.type Article en


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