Dynamical Evolution of the RS CVn-type Binaries
dc.contributor.author | Demircan, Osman | |
dc.date.accessioned | 2025-01-27T19:02:42Z | |
dc.date.available | 2025-01-27T19:02:42Z | |
dc.date.issued | 1999 | |
dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
dc.description.abstract | The orbital angular momentum (orbital AM) of a sample of forty RS CVn-type binaries with the orbital periods P?10 days were estimated and the orbital AM distribution with respect to P was critically interpreted as the orbital AM evolution of these systems caused by the magnetic breaking process with the existence of spin-orbit coupling. The empirical relations (between the orbital AM loss, mass loss and period variation) derived from the diagram of the orbital AM distribution were used in deriving a semi-empirical formula for the dynamical evolution of the RS CVn-type binaries. The magnetic breaking induced dynamical evolution of the RS CVn-type binaries maybe at different rates but is always towards the shorter periods in the existence of spin-orbit coupling and before the Roche lobe filling of a component star. | |
dc.identifier.endpage | 432 | |
dc.identifier.issn | 1300-0101 | |
dc.identifier.issue | 2 | |
dc.identifier.scopus | 2-s2.0-0348226531 | |
dc.identifier.scopusquality | Q2 | |
dc.identifier.startpage | 425 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12428/13638 | |
dc.identifier.volume | 23 | |
dc.indekslendigikaynak | Scopus | |
dc.language.iso | en | |
dc.relation.ispartof | Turkish Journal of Physics | |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.snmz | KA_Scopus_20250125 | |
dc.title | Dynamical Evolution of the RS CVn-type Binaries | |
dc.type | Article |