Radiation-driven winds in binary X-ray source systems

Details Radiation-driven winds in binary X-ray source systems Radiation-driven winds in binary X-ray source systems

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978cosp.meets....m&link_type=abstract

COSPAR, Plenary Meeting, 21st, Innsbruck, Austria, May 29-June 10, 1978, Paper. 8 p.

Physics

Binary Stars, Stellar Winds, X Ray Sources, Early Stars, Stellar Gravitation, Stellar Mass Accretion, Velocity Distribution, Wind Velocity

Scientific paper

The hydrodynamics of line-driven stellar winds in binary systems containing a weak X-ray source is investigated. The gravitational, ionization, and heating effects due to the secondary on the acceleration of the wind are taken into account. It is found that the changes in the acceleration which result from the presence of even a weak X-ray source can profoundly alter the wind velocity profile.

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