? Scuti-type pulsation in the hot component of the Algol-type binary system BG Peg
dc.contributor.author | Senyuz, T. | |
dc.contributor.author | Soydugan, Esin | |
dc.date.accessioned | 2025-01-27T21:06:11Z | |
dc.date.available | 2025-01-27T21:06:11Z | |
dc.date.issued | 2014 | |
dc.department | Çanakkale Onsekiz Mart Üniversitesi | |
dc.description | 301st Symposium of the International-Astronomical-Union -- AUG 19-23, 2013 -- Wroclaw, POLAND | |
dc.description.abstract | In 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.sponsorship | Int 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.sponsorship | Turkish Scientific and Technical Research Council [107T634] | |
dc.description.sponsorship | We wish to thank the Turkish Scientific and Technical Research Council (Grant no. 107T634) for supporting this study. | |
dc.identifier.doi | 10.1017/S1743921313015160 | |
dc.identifier.endpage | 484 | |
dc.identifier.isbn | 978-1-10704-517-0 | |
dc.identifier.issn | 1743-9213 | |
dc.identifier.issn | 1743-9221 | |
dc.identifier.issue | 301 | |
dc.identifier.scopus | 2-s2.0-84894548531 | |
dc.identifier.scopusquality | Q4 | |
dc.identifier.startpage | 483 | |
dc.identifier.uri | https://doi.org/10.1017/S1743921313015160 | |
dc.identifier.uri | https://hdl.handle.net/20.500.12428/27922 | |
dc.identifier.volume | 9 | |
dc.identifier.wos | WOS:000450807000116 | |
dc.identifier.wosquality | N/A | |
dc.indekslendigikaynak | Web of Science | |
dc.indekslendigikaynak | Scopus | |
dc.language.iso | en | |
dc.publisher | Cambridge Univ Press | |
dc.relation.ispartof | Precision Asteroseismology | |
dc.relation.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.snmz | KA_WoS_20250125 | |
dc.subject | techniques: photometric | |
dc.subject | stars: binaries: eclipsing | |
dc.subject | stars: individual (BG Peg) | |
dc.title | ? Scuti-type pulsation in the hot component of the Algol-type binary system BG Peg | |
dc.type | Conference Object |