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 |
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dc.format.mimetype |
application/pdf |
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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 |