The nonthermal radio emission of binary stars with relativistic components

Details The nonthermal radio emission of binary stars with relativistic components The nonthermal radio emission of binary stars with relativistic components

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1189l&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Nov.-Dec. 1987, p. 1189-1198. In Russian.

Astronomy and Astrophysics

Astronomy

4

Binary Stars, Neutron Stars, Nonthermal Radiation, Radio Emission, Relativistic Theory, Stellar Mass Ejection, Thermal Emission, B Stars, O Stars, Refracted Waves, Stellar Models, Stellar Winds

Scientific paper

The article is devoted to an analysis of possible manifestations of ejecting neutron stars in double systems with normal companions. For the first time, the problem of the propagation of radio emission from a point source orbiting in the stellar wind of the optical star is solved accounting for refraction. In the framework of this model, an attempt is made to explain the recently detected nonthermal radio emission from some OB stars.

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