Ionization effects in the radiative driving of stellar winds in massive X ray binary systems

Details Ionization effects in the radiative driving of stellar winds in massive X ray binary systems Ionization effects in the radiative driving of stellar winds in massive X ray binary systems

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..621s&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 621-625 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

Ionization, Stellar Mass Ejection, Stellar Physics, Stellar Winds, X Ray Astronomy, X Ray Binaries, Neutron Stars, Radiative Transfer, Stellar Atmospheres, Stellar Mass Accretion, Stellar Structure, Stellar Temperature

Scientific paper

Massive X ray binaries consist of an early type primary lossing mass via a strong stellar wind driven by the stars radiation field, and an accreting neutron star companion. The X rays from the neutron star affect the wind dynamics by changing the temperature and ionization structure. The effect of the accretion powered X rays on the radiative line force that drives the stellar wind is calculated. The consequences of these calculations for the wind dynamics in massive X ray binaries is discussed.

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