Starspot trek: The motion picture

IF 0.4 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS

Contributions of the Astronomical Observatory Skalnate Pleso Pub Date : 2020-04-06 DOI:10.31577/caosp.2020.50.2.490

B. Debski

引用次数: 1

Abstract

The longitudinal spot migration can be traced with the observation of the O’Connell effect and maxima separation variations. Judging by the correlations between the light curve parameters, the migration processes are confined to the polar regions of the more massive star in a contact binary.

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《星际迷航:电影》

通过观察O 'Connell效应和最大分离变化，可以追踪到斑的纵向迁移。根据光曲线参数之间的相关性判断，迁移过程仅限于接触双星中质量较大的恒星的极区。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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来源期刊

Contributions of the Astronomical Observatory Skalnate Pleso 地学天文-天文与天体物理

CiteScore

1.10

自引率

20.00%

发文量

审稿时长

>12 weeks

期刊介绍： Contributions of the Astronomical Observatory Skalnate Pleso" (CAOSP) is published by the Astronomical Institute of the Slovak Academy of Sciences (SAS). The journal publishes new results of astronomical and astrophysical research, preferentially covering the fields of Interplanetary Matter, Stellar Astrophysics and Solar Physics. We publish regular papers, expert comments and review contributions.