Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.103....1s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 103, no. 1, Aug. 1984, p. 1-7.
Astronomy and Astrophysics
Astrophysics
2
Binary Stars, Neutron Stars, Peculiar Stars, Stellar Models, X Ray Sources, X Ray Stars, Astronomical Models, Gamma Rays, Infrared Radiation, Light Curve, Pulsars, Stellar Mass Accretion
Scientific paper
A model of Cyg X-3, as a binary cocooned star system with two sources of X-rays, one above the polar caps of the neutron star - the usual pulsar radiation - and the other around the equatorial plane of the magnetobounding surface formed due to the interaction of the infalling plasma and the magnetic field of the neutron star, is made. The X-ray, gamma-ray, and IR radiation light curves are considered from the shadow effect. An upper limit on the mass of the neutron star is estimated from the consideration of periodic derivative purely due to mass loss. A comparison is made with the results of Elsner et al. (1980) and Ghosh et al. (1981), which they derived from the consideration of the period derivative purely from apsidal motion.
Duorah Hira Lal
Manihar Singh L.
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