Dergiler / Bitlis Eren University Journal of Science and Technology / 2020 / Cilt: 10 - Sayı: 2

Orbital period behaviour of three semi-detached binaries AI Cru, V1898 Cyg and Z Vul

Sayfa
49–53
Yayın Tarihi
2020-12-28
DOI
—
🏛️Bu makalenin bibliyografik verileri ve tam metin bağlantısı DergiPark üzerinden sağlanmıştır.
DergiPark Kaydı ↗
✨

Yapay Zeka Hızlı Bakış & Çıkarımlar

AI Insight
⚡ TL;DR(1 Cümlede Hızlı Çıkarım)

The minimum mass of probable tertiary components around AI Cru and V1898 Cyg were found to be 0.38 M⊙ and 0.26 M⊙, respectively.

📌 3 Maddede Bu Makale

🎯
Amaç & Hipotez:In this research, orbital period variation of three semi-deteached binaries AI Cru, V1898 Cyg and Z Vul investigated using all published eclipse times.
📊
Temel Bulgular & Veri:O-C analysis method has preferred as the method and the orbital periods of all systems are determined to increase.
💡
Sonuç & Katkı:The minimum mass of probable tertiary components around AI Cru and V1898 Cyg were found to be 0.38 M⊙ and 0.26 M⊙, respectively.
🔬Tür:Araştırma Makalesi
📍Kapsam:Genişletilmiş Akademik Örneklem
⚙️Değişkenler:Stars: eclipsing binaries · Semi-deteached binaries · Orbital period analysis

Abstract

In this research, orbital period variation of three semi-deteached binaries AI Cru, V1898 Cyg and Z Vul investigated using all published eclipse times. O-C analysis method has preferred as the method and the orbital periods of all systems are determined to increase. The changing rate of their period has been determined to be 0.8, 4.1 and 0.8 s/century for AI Cru, V1898 Cyg and Z Vul, respectively. Mass transfer between components has proposed as the cause of orbital period increase. For AI Cru, V1898 Cyg and Z Vul, mass transfer from less massive component to more massive and mass transfer rate was found to be 2.9×10-7, 1.5×10-7 and 5.3×10-8 M⊙/year respectively. Cyclic change has also seen in AI Cru and V1898 Cyg with increasing parabolic change. Cyclic periodic changes can be explained as being the result of a light-travel time effect via a tertiary body around the eclipsing pair. The minimum mass of probable tertiary components around AI Cru and V1898 Cyg were found to be 0.38 M⊙ and 0.26 M⊙, respectively.

🔖

Bu Makaleye Atıf Yap

YILDIRIM, M. F. (2020). Orbital period behaviour of three semi-detached binaries AI Cru, V1898 Cyg and Z Vul. Bitlis Eren University Journal of Science and Technology, Cilt: 10 - Sayı: 2, 49–53. https://ajindex.com/articles/743743

📄 Tam Metin PDF Okuyucu

📄

PDF görüntüleyici hazırlanıyor...

Kaynakça (1)

  1. Abt, H. A., Levy, S. G. and Gandet, T. L., 1972. Radial velocities of 65 early-type stars. Astronomical Journal, 77, 138. Applegate, J.H., 1992. A Mechanism for Orbital Period Modulation in Close Binaries, Astrophysical Journal, 385, 621. Astbury, T. H., 1909. The Algol Variable Z (26.1900) Vulpeculae. Astronomische Nachrichten, 182, 389. Bell, S. A., Kilkenny, D. and Malcolm, G. J. 1987. A photometric and spectroscopic study of the early-type binary AI Crucis. Monthly Notices of the Royal Astronomical Society, 226, 879. Caton, D. B. and Smith, A. B., 2005. Discovery of True Period and Solution of the Light Curve for V1898 Cygni. Bulletin of the American Astronomical Society, 37, 1169. Dervisoglu, A., Çakirli, Ö., Ibanoglu, C. and Sipahi, E., 2011. V1898 Cygni: An interacting eclipsing binary in the vicinity of North America nebula. Revista Mexicana de Astronomía y Astrofísica, 47, 297. Ghoreyshi, S. M. R., Ghanbari, J. and Salehi, F., 2008. Reanalysis of two eclipsing binaries: EE Aqr and Z Vul. Astrophysics and Space Science, 314, 331. Giuricin, G., Mardirossian, F., Mezzetti, M. and Predolin, F. 1980. Revised Photometric Elements of the Eclipsing Binary Ai-Crucis. Astrophysics and Space Science, 71, 411. Halbedel, E. M., 1985. HD 200776: a New Eclipsing Binary in Cygnus. Information Bulletin on Variable Stars, 2663, 1. Kopal, Z., 1959. Close Binary Stars; Double Stars. The International Astrophysics Series. Kreiner, J. M. and Ziolkowski, J., 1978. Period changes and evolutionary status of 18 Algoltype systems. Acta Astronomica, 28, 497. Kreiner, J.M., Kim, C-H., Nha, II-Seong, 2001. An atlas of O-C Diagrams of Eclipsing Binary Stars, Cracow, Poland. Lazaro, C., Arevalo, M. J. And Almenara, J. M., 2009. Absolute parameters of the Algol binary Z Vul. New Astronomy, 14, 528. Levato, H., 1975. Rotational velocities and spectral types for a sample of binary systems. Astronomy and Astrophysics, Supplement Series, 19, 91. Ollongren, A. 1956. Bulletin of the Astronomical Institutes of the Netherlands. 12, 313. Oosterhoff, P. Th. 1933. Bulletin of the Astronomical Institutes of the Netherlands. 9, 73. Paschke, A., Brat, L., 2006. O-C Gateway, a Collection of Minima Timings. Open European Journal on Variable Stars, 23, 13. Popper, D. M., 1957. Rediscussion of Eclipsing Binaries. III. Z Vulpeculae. Astrophysical Journal, 126, 53. Russo, G. 1981. Ai-Crucis - a Semi Detached System? Astrophysics and Space Science, 77, 197. Wesselink, A. J., 1969. Photometry of NGC 4