ANGULAR MOMENTUM EVOULUTION OF INTERACTING BINARY STAR SYSTEMS

dc.contributor.authorDemircan, Osman
dc.date.accessioned2025-01-27T21:21:59Z
dc.date.available2025-01-27T21:21:59Z
dc.date.issued2005
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractThe orbital angular momentum distribution of interacting binary star systems and the important role of mass loss and the Alfven radius in effective spin down and orbital shrinkage (and thus in the orbital angular momentum evolution) of these systems are reviewed.
dc.identifier.endpage251
dc.identifier.issn1313-0927
dc.identifier.issn2367-9522
dc.identifier.startpage248
dc.identifier.urihttps://hdl.handle.net/20.500.12428/29128
dc.identifier.volume20
dc.identifier.wosWOS:000433728700041
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.language.isoen
dc.publisherBulgarian Acad Sciences, Space Research & Technology Inst- Srti-Bas
dc.relation.ispartofAerospace Research in Bulgaria
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.titleANGULAR MOMENTUM EVOULUTION OF INTERACTING BINARY STAR SYSTEMS
dc.typeArticle

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