One less puzzle in Beta Lyrae?

Astronomy and Astrophysics – Astrophysics

Scientific paper

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B Stars, Binary Stars, Emission Spectra, Massive Stars, Absorption Spectra, Charge Coupled Devices, Stellar Envelopes, Stellar Models

Scientific paper

While it is clear that the emission-line object Beta Lyr A is a binary system, the nature of its more massive (but spectroscopically undetected) companion has been a mystery. It is suggested that the weak absorption lines of SiII at 6347 and 6371 A, which were recently discovered in CCD spectra of Beta Lyr to move in the opposite sense to the lines of the known B8II star, are not the photospheric lines of the companion but shell lines originating in the outer parts of a disk around that companion. This model seems to reconcile all the relevant observational data and opens the way to real progress in understanding the basic geometry of the system. One direct consequence of the model - if it is correct - is that the mysterious object inside the disk may be an essentially normal star with a mass and radius corresponding to a B0-B2V star.

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