A possible giant planet orbiting the cataclysmic variable LX Ser
文献类型:期刊论文
作者 | Li, Kai1,2![]() |
刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
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出版日期 | 2017-04-01 |
卷号 | 69期号:2 |
关键词 | binaries: eclipsing novae, cataclysmic variables stars: individual (LX Ser) |
ISSN号 | 0004-6264 |
DOI | 10.1093/pasj/psw134 |
文献子类 | Article |
英文摘要 | LX Ser is a deeply eclipsing cataclysmic variable with an orbital period of 0.1584325 d. 62 new eclipse times were determined by our observations and the AAVSO International Data base. Combining all available eclipse times, we analyzed the O-C behavior of LX Ser. We found that the O-C diagram of LXSer shows a sinusoidal oscillation with a period of 22.8 yr and an amplitude of 0.00035 d. Two mechanisms (i.e., the Applegate mechanism and the light-travel time effect) are applied to explain the cyclic modulation. We found that it is difficult to apply the Applegate mechanism to explain the cyclic oscillation in the orbital period. Therefore, the cyclic period change is most likely to be caused by the light-travel time effect due to the presence of a third body. The mass of the tertiary component was determined to be M-3 similar to 7.5M(Jup). We supposed that the tertiary companion is plausibly a giant planet. The stability of the giant planet was checked, and we found that the multiple system is stable. |
学科主题 | 天文学 ; 恒星与银河系 |
URL标识 | 查看原文 |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
WOS关键词 | STEPANYANS STAR ; CLOSE BINARIES ; PERIOD CHANGES ; NN-SER ; RS CVN ; DWARF ; EVOLUTION ; PHOTOMETRY ; COMPANION ; HERCULIS |
资助项目 | National Natural Science Foundation of China[U1431105] ; National Natural Science Foundation of China[11333002] ; Chinese Academy of Sciences[U1431105] ; Natural Science Foundation of Shandong Province[ZR2014AQ019] ; Young Scholars Program of Shandong University, Weihai[2016WHWLJH07] ; Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects[OP201303] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000401118500014 |
出版者 | OXFORD UNIV PRESS |
资助机构 | National Natural Science Foundation of China[U1431105, 11333002] ; Chinese Academy of Sciences[U1431105] ; Natural Science Foundation of Shandong Province[ZR2014AQ019] ; Young Scholars Program of Shandong University, Weihai[2016WHWLJH07] ; Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects[OP201303] |
源URL | [http://ir.ynao.ac.cn/handle/114a53/10066] ![]() |
专题 | 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Li, Kai |
作者单位 | 1.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai 264209, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China 3.School of Astronomy and Space Science and Key Laboratory ofModern Astronomy and Astrophysics in Ministry of Education, Nanjing University, Nanjing 210093, China |
推荐引用方式 GB/T 7714 | Li, Kai,Hu, Shaoming,Zhou, Jilin,et al. A possible giant planet orbiting the cataclysmic variable LX Ser[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2017,69(2). |
APA | Li, Kai.,Hu, Shaoming.,Zhou, Jilin.,Wu, Donghong.,Guo, Difu.,...&Wang, Xianyu.(2017).A possible giant planet orbiting the cataclysmic variable LX Ser.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,69(2). |
MLA | Li, Kai,et al."A possible giant planet orbiting the cataclysmic variable LX Ser".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 69.2(2017). |
入库方式: OAI收割
来源:云南天文台
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