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X-ray binary Beta Lyrae and its donor component structure
Published online by Cambridge University Press: 30 December 2019
Abstract
We show that the structure of magnetized accretion gas flows between the components of the Beta Lyrae system can cause a scattering gas shell that masks completely these components in soft X-ray region. Also we have calculated the inner structure of the donor that is filling a Roche lobe and is preceding a forming of the degenerate dwarf. We show that mass of the degenerate core of the donor is in region 0.3−0.5M⊙.
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- © International Astronomical Union 2019
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