dc.contributor.author | Çördük, Meryem | |
dc.contributor.author | Güver, Tolga | |
dc.contributor.author | Ülgen, Eyüp Kaan | |
dc.contributor.author | Yelkenci, Fuat Korhan | |
dc.contributor.author | Fişek, Süleyman | |
dc.contributor.author | Gündüz, Rahmi | |
dc.contributor.author | Göktürk, Fatih Erkam | |
dc.contributor.author | Özgüllü, Olcaytuğ | |
dc.contributor.author | Özgül, Görkem | |
dc.contributor.author | Sağlam, Mustafa Turan | |
dc.contributor.author | Aliş, Sinan | |
dc.date.accessioned | 2022-07-04T13:35:30Z | |
dc.date.available | 2022-07-04T13:35:30Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | Sağlam M. T. , Çördük M., Aliş S., Özgül G., Özgüllü O., Göktürk F. E. , Gündüz R., Fişek S., Yelkenci F. K. , Ülgen E. K. , et al., "Discovery of a Short Period Pulsator from Istanbul University Observatory", Turkish Journal of Astronomy and Astrophysics, cilt.3, sa.1, ss.8-16, 2022 | |
dc.identifier.issn | 2757-7295 | |
dc.identifier.other | av_502106e8-7aac-460d-bd0d-250715fb5122 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/182725 | |
dc.identifier.uri | https://doi.org/10.55064/tjaa.1103590 | |
dc.identifier.uri | https://avesis.istanbul.edu.tr/api/publication/502106e8-7aac-460d-bd0d-250715fb5122/file | |
dc.description.abstract | We report the discovery of a new short period pulsating variable in the field of exoplanet host star XO-2. Variable has been identified while it was being used as a comparison. In order to verify the variability of the candidate, a comprehensive follow-up was carried out. Period analysis of multi-band light curves revealed a very prominent and consistent pulsation periodicity ofP∼0.95" role="presentation" style="display: inline-block; line-height: 0; font-size: 17.219999313354492px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; margin: 0px; padding: 1px 0px; caret-color: rgb(17, 17, 17); color: rgb(17, 17, 17); font-family: Poppins; position: relative;">P∼0.95hours. Given the variability period, amplitude and the color index, the object is most likely a emph{delta Scuti} type variable. Absolute magnitude (Mv" role="presentation" style="display: inline-block; line-height: 0; font-size: 17.219999313354492px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; margin: 0px; padding: 1px 0px; caret-color: rgb(17, 17, 17); color: rgb(17, 17, 17); font-family: Poppins; position: relative;">Mv) and the color index(B−V)0" role="presentation" style="display: inline-block; line-height: 0; font-size: 17.219999313354492px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; margin: 0px; padding: 1px 0px; caret-color: rgb(17, 17, 17); color: rgb(17, 17, 17); font-family: Poppins; position: relative;">(B−V)0of the star determined as2.76" role="presentation" style="display: inline-block; line-height: 0; font-size: 17.219999313354492px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; margin: 0px; padding: 1px 0px; caret-color: rgb(17, 17, 17); color: rgb(17, 17, 17); font-family: Poppins; position: relative;">2.76and0.22" role="presentation" style="display: inline-block; line-height: 0; font-size: 17.219999313354492px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; margin: 0px; padding: 1px 0px; caret-color: rgb(17, 17, 17); color: rgb(17, 17, 17); font-family: Poppins; position: relative;">0.22, respectively. This(B−V)0" role="presentation" style="display: inline-block; line-height: 0; font-size: 17.219999313354492px; word-wrap: normal; white-space: nowrap; float: none; direction: ltr; max-width: none; max-height: none; min-width: 0px; min-height: 0px; border: 0px; margin: 0px; padding: 1px 0px; caret-color: rgb(17, 17, 17); color: rgb(17, 17, 17); font-family: Poppins; position: relative;">(B−V)0of the star corresponds to A7 spectral type with an approximate effective temperature of 7725 K. Machine-learning analysis of the time-series data also revealed that the object is of variable type DSCT with a probability of 78%. | |
dc.language.iso | tur | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Multidisciplinary | |
dc.subject | Physics and Astronomy (miscellaneous) | |
dc.subject | Temel Bilimler | |
dc.subject | Physical Sciences | |
dc.subject | Astronomy and Astrophysics | |
dc.subject | General Physics and Astronomy | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Doğa Bilimleri Genel | |
dc.subject | Uzay bilimi | |
dc.subject | Fizik | |
dc.subject | ÇOK DİSİPLİNLİ BİLİMLER | |
dc.title | Discovery of a Short Period Pulsator from Istanbul University Observatory | |
dc.type | Makale | |
dc.relation.journal | Turkish Journal of Astronomy and Astrophysics | |
dc.contributor.department | İstanbul Üniversitesi , Fen Fakültesi , Astronomi Ve Uzay Bilimleri Bölümü | |
dc.identifier.volume | 3 | |
dc.identifier.issue | 1 | |
dc.identifier.startpage | 8 | |
dc.identifier.endpage | 16 | |
dc.contributor.firstauthorID | 3433132 | |