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Pulsations in Cool Eclipsing Binary System V699 Cyg

Azizbek MatekovUlugh Beg Astronomical Institute of the Uzbekistan Academy of Science., University of the Chinese Academy of Sciences, Yuquan Road 19, Beijing, 100049, Sijingshang Block, P.R. China., Yunnan Observatories of Chinese Academy of Sciences, P.O. Box 110, Kunming, 650011, ChinaA. S. HojaevUlugh Beg Astronomical Institute of the Uzbekistan Academy of ScienceО. БурхоновUlugh Beg Astronomical Institute of the Uzbekistan Academy of Science

Zenodo (CERN European Organization for Nuclear Research)repository2022en

ABI

Annotatsiya

<pre>Abstract. Aims: We aimed to perform the analysis of the long-term variability and precession of the orbital inclination of the eclipsing binary system V699 Cyg for the first time. Methods: We obtained the long-term photometric observation series of the eclipsing binary system V699 Cyg at High-altitude Maidanak Astrophysical Observatory in Uzbekistan and performed the deep analysis of the light curves of V699 Cyg. Results: We found that the system changed the orbital inclination. At the same time within eclipse the object periodically changes its brightness with a small amplitude (∼ 0.037mag) within the eclipse. Based on analysis of the all light curves available, we have found that V699 Cyg also exhibit the periodic pulsating oscillations.</pre>

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Mavzular

Astrophysical Phenomena and Observations Astronomical Observations and Instrumentation Astronomy and Astrophysical Research

Identifikatorlar

DOI: 10.5281/zenodo.7579686

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