| 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 |