The Self-Consistent Model of the Be Star Envelope and the Source of the Be-star X-ray Luminosity

Details The Self-Consistent Model of the Be Star Envelope and the Source of the Be-star X-ray Luminosity The Self-Consistent Model of the Be Star Envelope and the Source of the Be-star X-ray Luminosity

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..92k&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 92-92"

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Using a self-consistent gasdynamical model, we carried out a numerical modeling of the envelopes of Be stars in binary systems. The model can explain the formation of Be-star envelopes in the detached binary systems for the B-star primaries having rotational velocities below breakup. Numerical modeling for three different Be stars was performed. It was found that the mass transfer rates via the inner Lagrangian point can be large enough to generate the X-ray luminosity observed for the Be/X binaries. Numerical computations confirm the observed correlation of the X-ray luminosity and orbital period in the Be/X binaries.

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