? Scuti-type pulsation in the hot component of the Algol-type binary system BG Peg

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dc.contributor.authorSenyuz, T.
dc.contributor.authorSoydugan, Esin
dc.date.accessioned2025-01-27T21:06:11Z
dc.date.available2025-01-27T21:06:11Z
dc.date.issued2014
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description301st Symposium of the International-Astronomical-Union -- AUG 19-23, 2013 -- Wroclaw, POLAND
dc.description.abstractIn this study, 23 Algol-type binary systems, which were selected as candidate binaries with pulsating components, were observed at the canakkale Onsekiz Mart University Observatory. One of these systems was BG Peg. Its hotter component shows delta Scuti-type light variations. Physical parameters of BG Peg were derived from modelling the V light curve using the Wilson-Devinney code. The frequency analysis shows that the pulsational component of the BG Peg system pulsates in two modes with periods of 0.039 and 0.047 d. Mode identification indicates that both modes are most likely non-radial l = 2 modes.
dc.description.sponsorshipInt Astron Union Div G Stars & Stellar Phys,Int Astron Union Commiss No 27 Variable Stars,Int Astron Union Commiss No 35 Stellar Constitut,Ministerstwo Nauki Szkolnictwa Wyzszego,Fundacja Astronomii Polskiej M Kopernika,Int Astron Union
dc.description.sponsorshipTurkish Scientific and Technical Research Council [107T634]
dc.description.sponsorshipWe wish to thank the Turkish Scientific and Technical Research Council (Grant no. 107T634) for supporting this study.
dc.identifier.doi10.1017/S1743921313015160
dc.identifier.endpage484
dc.identifier.isbn978-1-10704-517-0
dc.identifier.issn1743-9213
dc.identifier.issn1743-9221
dc.identifier.issue301
dc.identifier.scopus2-s2.0-84894548531
dc.identifier.scopusqualityQ4
dc.identifier.startpage483
dc.identifier.urihttps://doi.org/10.1017/S1743921313015160
dc.identifier.urihttps://hdl.handle.net/20.500.12428/27922
dc.identifier.volume9
dc.identifier.wosWOS:000450807000116
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherCambridge Univ Press
dc.relation.ispartofPrecision Asteroseismology
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20250125
dc.subjecttechniques: photometric
dc.subjectstars: binaries: eclipsing
dc.subjectstars: individual (BG Peg)
dc.title? Scuti-type pulsation in the hot component of the Algol-type binary system BG Peg
dc.typeConference Object

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