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On the period variation of the WUMa-type contact binary V502 Ophiuchi
Liu QY(刘清耀); Yang YL(杨毓兰); Liu, QY (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
2006
卷号6期号:3页码:331-337
DOI10.1088/1009-9271/6/3/08
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收录类别SCI
关键词Stars : Contact Binary Period Change Star : Individual : V502 Oph
摘要The variation in the orbital period of the W UMa type contact binary V502 Oph is analyzed. The orbital period exhibits a wavelike variation with a periodicity of 23.0 years and an amplitude of Delta P = 1.24 x 10(-6) days superimposed on secular decrease of dP/dt = 1.68 x 10(-7) day per year. The long-term decrease may be accompanied by the contraction of the secondary at a rate of 83 m per year and a mass transfer rate from the primary to the secondary of 4.28 x 10(-8) M-. per year. The short-term oscillation may be explained by the presence of a third component. Orbital elements of the third body and its possible mass are presented.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1009-9271
URL查看原文
归档日期2006-08-07
WOS记录号WOS:000238416500008
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]URSAE MAJORIS SYSTEMS ; PHOTOELECTRIC OBSERVATIONS ; STARS
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被引频次:5[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/4208
专题其他
通讯作者Liu, QY (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011
第一作者单位中国科学院云南天文台
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Liu QY,Yang YL,Liu, QY . On the period variation of the WUMa-type contact binary V502 Ophiuchi[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2006,6(3):331-337.
APA Liu QY,Yang YL,&Liu, QY .(2006).On the period variation of the WUMa-type contact binary V502 Ophiuchi.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,6(3),331-337.
MLA Liu QY,et al."On the period variation of the WUMa-type contact binary V502 Ophiuchi".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 6.3(2006):331-337.
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