KIC7739728—A New FK Com-Type Star Candidate
- Авторлар: Savanov I.S.1
-
Мекемелер:
- Institute of Astronomy of the Russian Academy of Sciences
- Шығарылым: Том 74, № 3 (2019)
- Беттер: 288-292
- Бөлім: Article
- URL: https://journals.rcsi.science/1990-3413/article/view/212948
- DOI: https://doi.org/10.1134/S1990341319030052
- ID: 212948
Дәйексөз келтіру
Аннотация
We present a study of the parameters of objects belonging to a sparsely populated group of FKCom-type stars, as well as a brief review of our earlier studies dedicated to the search for stellar candidates of this type. We consider the data for another new candidate-the star KIC 7739728. The light curve of this star clearly demonstrates properties of regular rotational modulation, the rotation exhibits a differential nature (the parameter ΔΩ = 0.010 rad day-1), a flip-flop effect is observed in the positions of active longitudes, as well as cyclic variations of the spot positions on the star’s surface.
Негізгі сөздер
Авторлар туралы
I. Savanov
Institute of Astronomy of the Russian Academy of Sciences
Хат алмасуға жауапты Автор.
Email: isavanov@inasan.rssi.ru
Ресей, Moscow, 119017
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