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The ROSAT bright source 1RXS J201607.0+251645: an active Algol-type binary
Li, Hua-Li1,2,3; Yang, Yuan-Gui1,4; Su, Wei1,3; Wang, Hui-Juan1,3; Wei, Jian-Yan1
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2009-09-01
卷号9期号:9页码:1035-1048
关键词stars: binaries: close stars: binaries: eclipsing stars: individual: 1RXS J201607.0+251645, HD 339946
ISSN号1674-4527
通讯作者lhl@bao.ac.cn
英文摘要1RXS J201607.0+251645 is identified as an eclipsing binary. We present preliminary observations in the V band with the 0.6-m telescope for three years and extensive observations in the V and R bands with the 0.8-m telescope for six nights, respectively. The light curve of the system is EB type. Five light minimum times were obtained and the orbital period of 0.388058(d)(+/-0.00044(d)) is determined. The photometric solution given by the 2003-version of the Wilson-Devinney program suggests that the binary is a semidetached system with photometric mass ratio 0.895(+/-0.006), which is probably comprised of a G5 primary and an oversized K5 secondary. The less massive component has completely filled its Roche lobe, while the other one almost fills its Roche lobe with a filling factor of 93.4%. The system shows a varying O'Connell effect in its phase folded diagrams from 2005 to 2007, and is X-ray luminous with log L(X)/L(bol) similar to -3.27. Possible mechanisms to account for these two phenomena are discussed. Finally, we infer that the binary may be in thermal oscillation or may evolve into a contact binary.
学科主题恒星和恒星物理
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]ALL-SKY SURVEY ; MAGNETIC ACTIVITY ; LIGHT CURVES ; MASS-TRANSFER ; ORION NEBULA ; RS CVN ; STARS ; EVOLUTION ; SYSTEMS ; PERIOD
收录类别SCI
资助信息National Natural Science Foundation of China (Grant Nos. 10778707 and 10473013)
原文出处http://www.raa-journal.org
语种英语
WOS记录号WOS:000270404200008
公开日期2013-03-06
内容类型期刊论文
源URL[http://ir.xao.ac.cn/handle/45760611-7/195]  
专题新疆天文台_其它
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Chinese Acad Sci, Urumqi Observ, Natl Astron Observ, Urumqi 830011, Peoples R China
3.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
4.Huaibei Coal Ind Teachers Coll, Sch Phys & Elect Informat, Huaibei 235000, Peoples R China
推荐引用方式
GB/T 7714
Li, Hua-Li,Yang, Yuan-Gui,Su, Wei,et al. The ROSAT bright source 1RXS J201607.0+251645: an active Algol-type binary[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2009,9(9):1035-1048.
APA Li, Hua-Li,Yang, Yuan-Gui,Su, Wei,Wang, Hui-Juan,&Wei, Jian-Yan.(2009).The ROSAT bright source 1RXS J201607.0+251645: an active Algol-type binary.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,9(9),1035-1048.
MLA Li, Hua-Li,et al."The ROSAT bright source 1RXS J201607.0+251645: an active Algol-type binary".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 9.9(2009):1035-1048.
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