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Journals / Turkish Journal of Astronomy and Astrophysics / 2020 / Cilt: 1 Sayı: 3

Photometric solutions for three eclipsing binary systems: SY Sge, V688 Aql, and CY Ari

H.gökhan Gökay(ANKARA ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ)0000-0003-0264-6246
Derya Öztürk Çetni(ATATÜRK ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE ASTROFİZİK BÖLÜMÜ)0000-0003-1671-5193
Zahide Terzioğlu(ANKARA ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ)0000-0002-4507-7074
Sacit Özdemir(ANKARA ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ)0000-0002-0292-7059
Deniz Çoker(ANKARA ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ)0000-0003-3816-8709
Ceren Garner(ANKARA ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜ)
Pages
1–7
Publication Date
2020-12-31
DOI
—
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AI Summary & Key Takeaways

AI Insight
⚡ TL;DR(Too Long; Didn't Read)

Combining system parameters with photometric mass ratio allows us to obtain absolute parameters of the systems which leads to locate the systems on theoretical HR diagram and to estimate their evolutionary status.

📌 3 Key Takeaways

🎯
Objective & Hypothesis:We present a detailed light curve analysis of three eclipsing binaries, consisted of two Algol type systems, SY Sge and V688 Aql, and one W UMa type system, CY Ari, observed at the Ankara University Observatory.
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Key Findings & Data:Moreover, since there is not any radial velocity measurement of the systems, a q-search test was applied for all three systems to reach a minimized $\chi^2$.
💡
Conclusion & Impact:Combining system parameters with photometric mass ratio allows us to obtain absolute parameters of the systems which leads to locate the systems on theoretical HR diagram and to estimate their evolutionary status.
🔬Design:Araştırma Makalesi
📍Scope:Comprehensive Sample
⚙️Variables:eclipsing binaries · fundamental parameters · photometry

Abstract

We present a detailed light curve analysis of three eclipsing binaries, consisted of two Algol type systems, SY Sge and V688 Aql, and one W UMa type system, CY Ari, observed at the Ankara University Observatory. The light curves constructed in Johnson BVRI pass-bands were simultaneously analysed on the basis of Roche Geometry. Fourier coefficients method was applied on the light curve of W UMa type system to estimate a set of initial system parameters. Moreover, since there is not any radial velocity measurement of the systems, a q-search test was applied for all three systems to reach a minimized $\chi^2$. Combining system parameters with photometric mass ratio allows us to obtain absolute parameters of the systems which leads to locate the systems on theoretical HR diagram and to estimate their evolutionary status.

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Cite This Article

Gökay, H., Çetni, D. Ö., Terzioğlu, Z., Özdemir, S., Çoker, D., Garner, C. (2020). Photometric solutions for three eclipsing binary systems: SY Sge, V688 Aql, and CY Ari. Turkish Journal of Astronomy and Astrophysics, Cilt: 1 Sayı: 3, 1–7. https://ajindex.com/articles/1555460

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