Comprehensive analysis of the eclipsing binaries V527 Dra and V2846 Cyg
Monthly Notices of the Royal Astronomical Society, cilt.532, sa.3, ss.3582-3603, 2024 (SCI-Expanded, Scopus)
- Yayın Türü: Makale / Tam Makale
- Cilt numarası: 532 Sayı: 3
- Basım Tarihi: 2024
- Doi Numarası: 10.1093/mnras/stae1709
- Dergi Adı: Monthly Notices of the Royal Astronomical Society
- Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, Aerospace Database, Applied Science & Technology Source, Communication Abstracts, Compendex, INSPEC, Metadex, zbMATH, DIALNET, Civil Engineering Abstracts
- Sayfa Sayıları: ss.3582-3603
- Anahtar Kelimeler: binaries: close, binaries: eclipsing, stars: fundamental parameters, stars: individual: V2846 Cyg, stars: individual: V527 Dra
- Ankara Üniversitesi Adresli: Evet
Özet
This is the first comprehensive study of the eclipsing binaries V527 Dra and V2846 Cyg, based on radial velocities and ground- and space-based light curves. We perform detailed modeling of these data to derive the absolute parameters and the orbital properties of the two systems. V527 Dra is found to be a semidetached, and V2846 Cyg a contact binary. Both show continual out-of-eclipse variations that can be explained by migrating dark spots of magnetic origin. We also perform the eclipse timing variation (ETV) analysis which reveals that V527 Dra has a tertiary companion whose mass (∼1 M ⊙) and orbital inclination ( ∼70 °) are additionally constrained by radial velocities. The ETV diagram of V2846 Cyg displays a quadratic trend accompanied by a low-amplitude cyclic variation, likely due to a magnetic cycle, although further eclipse times are needed to provide a clearer explanation. Lastly, we demonstrate a correlation between the variations in spot parameters obtained via light curve modelling for individual orbital cycles and the residual ETVs, essentially confirming the assumption of magnetic activity in both systems.