V. V. Dyachenko, I. A. Yakunin, R. M. Bayazitov, S. A. Grigoriev, T. A. Ryabchikova, Yu. V. Pakhomov, E. A. Semenko, A. S. Beskakotov, A. A. Mitrofanova, A. F. Maksimov, Yu. Yu. Balega
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引用次数: 0
Abstract
We present a refined speckle-interferometric orbit of a binary system \(\mu\) Cet, with the main component studied based on the analysis of photometric and spectroscopic data, obtained with the SAO RAS 6-m telescope. The object was initially classified as a giant with chemical composition anomalies. As a result of our analysis, we conclude that the star belongs to the Main Sequence, to the class of non-peculiar stars. Analysis of photometric data from the TESS mission indicates that the main component of the system belongs to the \(\gamma\) Dor pulsators.
期刊介绍：
Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.
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