Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/131038
Title: The Role of Meridional Circulation in the Formation of Classical Be Stars
Authors: Staritsin, E. I.
Issue Date: 2023
Publisher: Pleiades Publishing
Citation: Staritsin, E 2023, 'The Role of Meridional Circulation in the Formation of Classical Be Stars', Astronomy Reports, Том. 67, № 9, стр. 959-962. https://doi.org/10.1134/S1063772923090123
Staritsin, E. (2023). The Role of Meridional Circulation in the Formation of Classical Be Stars. Astronomy Reports, 67(9), 959-962. https://doi.org/10.1134/S1063772923090123
Abstract: Abstract: At the stage of mass exchange in a binary system, the meridional circulation brings to the surface of the star up to two-thirds of the angular momentum that entered the star along with the accreted matter. As a result, the mass and angular momentum of the star can increase due to accretion. After the end of accretion, the star has a rotation typical of rapidly rotating Be stars. It is assumed that the angular momentum carried by the meridional circulation to the star’s surface from the accreted matter is removed from the star by the accretion disk. The article is based on a talk presented at the astrophysical memorial seminar “Novelties in Understanding the Evolution of Binary Stars,” dedicated to the 90th anniversary of Professor M.A. Svechnikov. © 2023, The Author(s).
Keywords: BE STARS
BINARY STAR SYSTEMS
STRUCTURE AND EVOLUTION OF STARS
URI: http://elar.urfu.ru/handle/10995/131038
Access: info:eu-repo/semantics/openAccess
cc-by
License text: https://creativecommons.org/licenses/by/4.0/
SCOPUS ID: 85179300701
WOS ID: 001122207000010
PURE ID: 49823074
ISSN: 1063-7729
DOI: 10.1134/S1063772923090123
Sponsorship: Ministry of Education and Science of the Russian Federation, Minobrnauka: FEUZ-2023-0019
This work was supported by the Ministry of Science and Higher Education of the Russian Federation, topic No. FEUZ-2023-0019.
Appears in Collections:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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