1. Электронный научный архив УрФУ
  2. 00. Общеуниверситетские коллекции
  3. Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC
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dc.contributor.authorStaritsin, E. I.en
dc.date.accessioned2024-04-05T16:37:25Z-
dc.date.available2024-04-05T16:37:25Z-
dc.date.issued2023-
dc.identifier.citationStaritsin, 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/S1063772923090123harvard_pure
dc.identifier.citationStaritsin, 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/S1063772923090123apa_pure
dc.identifier.issn1063-7729-
dc.identifier.otherFinal2
dc.identifier.otherAll Open Access, Hybrid Gold3
dc.identifier.otherhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85179300701&doi=10.1134%2fS1063772923090123&partnerID=40&md5=14298a9599ec8cdca832ace2333874741
dc.identifier.otherhttps://link.springer.com/content/pdf/10.1134/S1063772923090123.pdfpdf
dc.identifier.urihttp://elar.urfu.ru/handle/10995/131038-
dc.description.abstractAbstract: 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).en
dc.description.sponsorshipMinistry of Education and Science of the Russian Federation, Minobrnauka: FEUZ-2023-0019en
dc.description.sponsorshipThis work was supported by the Ministry of Science and Higher Education of the Russian Federation, topic No. FEUZ-2023-0019.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherPleiades Publishingen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.rightscc-byother
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/unpaywall
dc.sourceAstronomy Reports2
dc.sourceAstronomy Reportsen
dc.subjectBE STARSen
dc.subjectBINARY STAR SYSTEMSen
dc.subjectSTRUCTURE AND EVOLUTION OF STARSen
dc.titleThe Role of Meridional Circulation in the Formation of Classical Be Starsen
dc.typeArticleen
dc.typeinfo:eu-repo/semantics/articleen
dc.type|info:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1134/S1063772923090123-
dc.identifier.scopus85179300701-
local.contributor.employeeStaritsin, E.I., Kourovka Astronomical Observatory, Ural Federal University Named after the First President of Russia B.N. Yeltsin, Yekaterinburg, 623132, Russian Federationen
local.description.firstpage959-
local.description.lastpage962-
local.issue9-
local.volume67-
dc.identifier.wos001122207000010-
local.contributor.departmentKourovka Astronomical Observatory, Ural Federal University Named after the First President of Russia B.N. Yeltsin, Yekaterinburg, 623132, Russian Federationen
local.identifier.pure49823074-
local.identifier.eid2-s2.0-85179300701-
local.identifier.wosWOS:001122207000010-
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