中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
YY Geminorum: A very late type close binary with possible magnetic stellar wind

文献类型:期刊论文

作者Qian SB(钱声帮)1,2; Liu, DL3; Tan, WL4; Soonthornthum, B5
刊名ASTRONOMICAL JOURNAL
出版日期2002-08
卷号124期号:2页码:1060-1063
关键词binaries : close stars : individual (YY Geminorum) stars : mass loss
ISSN号0004-6256
产权排序第一完成单位
通讯作者Qian, SB (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, POB 110, Kunming 650011, Peoples R China.
英文摘要The O-C curve of the very late type close binary (dMle+dMle)YY Geminorum is formed and analyzed based on all available times of minimum light. It is found that the orbital period shows a secular decrease with rate dP/dt = -1.08x10(-8) days yr(-1). There is weak evidence indicating that a small-amplitude period oscillation is superposed on the period decrease. YY Gem is a well-detached eclipsing binary containing two very active components. The secular period decrease may suggest that the system is undergoing secular mass and angular momentum loss via a magnetic stellar wind. If the small-amplitude oscillation is real, it can be explained either by magnetic activity cycles or by the presence of a giant planet or brown dwarf.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]ORBITAL PERIOD MODULATION ; STARS
收录类别SCI
原文出处http://iopscience.iop.org/1538-3881/124/2/1060/
语种英语
WOS记录号WOS:000176888900033
源URL[http://ir.ynao.ac.cn/handle/114a53/5756]  
专题云南天文台_双星与变星研究组
作者单位1.Yunnan Observatory, National Astronomical Observatories, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, China
2.United Laboratory of Optical Astronomy, Chinese Academy of Sciences
3.Nayong County Second Middle School, 553300 Nayong, Guizhou, China
4.Department of Physics, Guizhou Normal University, 550001 Guiyang, Guizhou, China
5.Department of Physics, Chiang Mai University, 50200 Chiang Mai, Thailand
推荐引用方式
GB/T 7714
Qian SB,Liu, DL,Tan, WL,et al. YY Geminorum: A very late type close binary with possible magnetic stellar wind[J]. ASTRONOMICAL JOURNAL,2002,124(2):1060-1063.
APA Qian SB,Liu, DL,Tan, WL,&Soonthornthum, B.(2002).YY Geminorum: A very late type close binary with possible magnetic stellar wind.ASTRONOMICAL JOURNAL,124(2),1060-1063.
MLA Qian SB,et al."YY Geminorum: A very late type close binary with possible magnetic stellar wind".ASTRONOMICAL JOURNAL 124.2(2002):1060-1063.

入库方式: OAI收割

来源:云南天文台

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