Ellipsoidal variability of symbiotic giants

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dc.creatorMikolajewska, J.
dc.creatorKolotilov, E. A.
dc.creatorShugarov, S. Yu.
dc.creatorTatarnikova, A. A.
dc.creatorYudin, B. F.
dc.date2002-10-22
dc.date.accessioned2026-07-25T18:48:03Z
dc.descriptionOne of fundamental questions in relation to symbiotic binaries is the process of mass transfer - Roche lobe overflow or stellar wind - and possibility of an accretion disc formation. The presence of secondary minima in the quiescent light curves of YY Her, CI Cyg and BF Cyg apparently due to ellipsoidal changes of the red giant provides here important clues.
dc.description4 pages, 2 figures. To appear in 'Symbiotic stars probing stellar evolution', eds. R.M.L. Corradi, J. Mikolajewska, T. Mahoney
dc.identifierhttps://arxiv.org/abs/astro-ph/0210492
dc.identifierhttp://arxiv.org/abs/astro-ph/0210492
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/58687
dc.subjectAstrophysics
dc.titleEllipsoidal variability of symbiotic giants
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