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Gasdynamical modelling of circumstellar matter in .beta. LyrA
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SYSNO ASEP 0124693 Document Type C - Proceedings Paper (int. conf.) R&D Document Type Conference Paper Title Gasdynamical modelling of circumstellar matter in .beta. LyrA Author(s) Bisikalo, D. V. (RU)
Boyarchuk, A. A. (RU)
Harmanec, Petr (ASU-R)
Hadrava, Petr (ASU-R) RID, ORCID
Kuznetsov, O. A. (RU)Source Title The Be phenomenon in early-type stars / Smith M. ; Henrichs H.F. ; Fabregat J.. - San Francisco : Astronomical Society of the Pacific, 2000 Pages s. 697-700 Number of pages 4 s. Action Colloquium of the International Astronomical Union /175./ Event date 28.06.1999-02.07.1999 VEvent location Alicante Country ES - Spain Language eng - English Country US - United States Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects IAA3003805 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR) CEZ AV0Z1003909 - ASU-R Annotation Available spectroscopic evidence of various circumstellar gaseous structures in the well-known binary .beta. Lyr in confronted with the results of 3-D gas-dynamical simulations of mass transfer between the binary components. It appears that the gas-dynamical model is capable to explain the formation of all basic observed components of the circumstellar matter, including the jet-like structures, recently found from interferometry and polarimetry of the object. Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2001
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