中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Photometric monitoring of the ROSAT selected late type stars

文献类型:期刊论文

作者Xing, L. F.; Zhang, X. B.; Wei, J. Y.
刊名NEW ASTRONOMY
出版日期2007-02-01
卷号12期号:4页码:346-352
关键词stars : late-type stars : pre-main sequence stars : rotation stars : spots
英文摘要We monitored the light variations of 16 solar-type stars recently discovered in the X-ray wave-length range during the ROSAT all-sky survey. We find that 9 out of 16 stars showed appreciable light variability with amplitudes of a few hundredths of a magnitude. They are all proved to be in periodic variations. Using the methods of the phase dispersion minimization (PDM) and Fourier Analysis (PERIOD04), we derive the photometric periods for these stars. The rotational periods are found range from 0.471 to 17.31 days and the period of stars most (of 7 stars) being shorter than 3 days. Apart from binaries system, the results give further evidence for the spin up of solar-type stars as predicted by models of angular momentum evolution of pre-main sequence stars. (c) 2006 Elsevier B.V. All rights reserved.
收录类别SCI
语种英语
WOS记录号WOS:000243609900006
源URL[http://ir.bao.ac.cn/handle/114a11/7292]  
专题国家天文台_光学天文研究部
作者单位1.Zhengzhou Univ Light Ind, Dept Technol & Phys, Zhengzhou 450002, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
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Xing, L. F.,Zhang, X. B.,Wei, J. Y.. Photometric monitoring of the ROSAT selected late type stars[J]. NEW ASTRONOMY,2007,12(4):346-352.
APA Xing, L. F.,Zhang, X. B.,&Wei, J. Y..(2007).Photometric monitoring of the ROSAT selected late type stars.NEW ASTRONOMY,12(4),346-352.
MLA Xing, L. F.,et al."Photometric monitoring of the ROSAT selected late type stars".NEW ASTRONOMY 12.4(2007):346-352.

入库方式: OAI收割

来源:国家天文台

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