Photometric and spectroscopic analysis of the eccentric eclipsing binary BD+72 780

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YILMAZ M., ÖZAVCI İ., BAHAR E., ŞENAVCI H. V., Azizoglu B.

Contributions of the Astronomical Observatory Skalnate Pleso, cilt.55, sa.3, ss.517-520, 2025 (SCI-Expanded)

• Yayın Türü: Makale / Tam Makale
• Cilt numarası: 55 Sayı: 3
• Basım Tarihi: 2025
• Doi Numarası: 10.31577/caosp.2025.55.3.517
• Dergi Adı: Contributions of the Astronomical Observatory Skalnate Pleso
• Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
• Sayfa Sayıları: ss.517-520
• Anahtar Kelimeler: eclipsing binary, radial velocity, stars
• Ankara Üniversitesi Adresli: Evet

Özet

In this study, we present the first radial velocity measurements of the eclipsing binary BD+72 780. We simultaneously modeled TESS light curves with our radial velocity data to derive the orbital and absolute parameters of the system. The analysis shows that the system is a detached binary with two different spectral types of components, and the orbit is slightly eccentric (e ∼ 0.07).