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δ Scuti-type pulsation in the hot component of the Algol-type binary system BG Peg
| Content Provider | Scilit |
|---|---|
| Author | Şenyüz, T. Soydugan, E. |
| Copyright Year | 2013 |
| Description | In this study, 23 Algol-type binary systems, which were selected as candidate binaries with pulsating components, were observed at the Çanakkale Onsekiz Mart University Observatory. One of these systems was BG Peg. Its hotter component shows δ 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. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/3552D26DC01F71F146BE49F6030B6CE6/S1743921313015160a.pdf/div-class-title-scuti-type-pulsation-in-the-hot-component-of-the-algol-type-binary-system-bg-peg-div.pdf |
| Ending Page | 484 |
| Page Count | 2 |
| Starting Page | 483 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921313015160 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S301 |
| Volume Number | 9 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2013-08-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics Photometric Eclipsing Individual (bg Peg) |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
