KIC7739728—A New FK Com-Type Star Candidate
- 作者: Savanov I.S.1
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隶属关系:
- Institute of Astronomy of the Russian Academy of Sciences
- 期: 卷 74, 编号 3 (2019)
- 页面: 288-292
- 栏目: Article
- URL: https://journals.rcsi.science/1990-3413/article/view/212948
- DOI: https://doi.org/10.1134/S1990341319030052
- ID: 212948
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详细
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.
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作者简介
I. Savanov
Institute of Astronomy of the Russian Academy of Sciences
编辑信件的主要联系方式.
Email: isavanov@inasan.rssi.ru
俄罗斯联邦, Moscow, 119017
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