Binary model of Circinus X-1. II - Radio emission

Details Binary model of Circinus X-1. II - Radio emission Binary model of Circinus X-1. II - Radio emission

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....87..299h&link_type=abstract

Astronomy and Astrophysics, vol. 87, no. 3, July 1980, p. 299-302.

Astronomy and Astrophysics

Astrophysics

21

Binary Stars, Radio Stars, Stellar Mass Ejection, Stellar Models, X Ray Sources, X Ray Stars, Absorption Spectra, Flares, Mass Transfer, Radio Emission, Stellar Luminosity, Stellar Magnetic Fields, Stellar Spectra, Stellar Winds

Scientific paper

A binary star model is used to account for the 16.5 d flaring behavior
of the radio emission from Circinus X-1. Mass transfer between the
primary star and the compact companion star triggers one or more
expanding Eddington luminosity-driven shocks in the vicinity of the
compact star which, in turn, produce radio emission.

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