中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Interactions between planets and evolved stars

文献类型:会议论文

作者Qian SB(钱声帮)1,2,3; Han ZT(韩忠涛)1,2,3; Fernández Lajús, E.4,5; Zhu LY(朱俐颖)1,2,3; Liao WP(廖文萍)1,2; Miloslav, Zejda6; Li LJ(李临甲)1,2; Voloshina, Irina7; Liu L(刘亮)1,2,3; He JJ(何家佳)1,2
出版日期2016-08-08
会议日期2015-12-14
会议地点Univ Hong Kong, Hong Kong, PEOPLES R CHINA
卷号728
期号4
DOI10.1088/1742-6596/728/4/042006
英文摘要

Searching for planetary companions to evolved stars (e.g., white dwarfs (WD) and Cataclysmic Variables (CV)) can provide insight into the interaction between planets and evolved stars as well as on the ultimate fate of planets. We have monitored decades of CVs and their progenitors including some detached WD binaries since 2006 to search for planets orbiting these systems. In the present paper, we will show some observational results of circumbinary planets in orbits around CVs and their progenitors. Some of our findings include planets with the shortest distance to the central evolved binaries and a few multiple planetary systems orbiting binary stars. Finally, by comparing the observational properties of planetary companions to single WDs and WD binaries, the interaction between planets and evolved stars and the ultimate fate of planets are discussed. © Published under licence by IOP Publishing Ltd.

源文献作者Kwok, S; Leung, KC
产权排序第1完成单位
资助机构Chinese Natural Science Foundation ; Yunnan Natural Science Foundation ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences
会议录Journal of Physics Conference Series - 11th Pacific Rim Conference on Stellar Astrophysics: Physics and Chemistry of the Late Stages of Stellar Evolution - Session III: Symbiotic Stars, Novae, and Binary Star Evolution
会议录出版者IOP PUBLISHING LTD
文献子类Proceedings Paper
学科主题天文学 ; 天体物理学
会议录出版地DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND
语种英语
URL标识查看原文
资助项目Chinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[11325315] ; Chinese Natural Science Foundation[11403095] ; Yunnan Natural Science Foundation[2014FB187] ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences[XDB09010202]
ISSN号1742-6588
WOS研究方向Astronomy & Astrophysics ; Physics
WOS记录号WOS:000397958000031
WOS关键词Common-envelope Binaries ; Orbital Period Distribution ; Main-sequence Binaries ; White-dwarf ; Eclipsing Binary ; Brown Dwarf ; Hu Aqr ; Cataclysmic Variables ; V2051 Ophiuchi ; Giant Planet
源URL[http://ir.ynao.ac.cn/handle/114a53/9798]  
专题云南天文台_双星与变星研究组
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Lajus, F
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, 650216 Kunming, P.R. China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P.O. Box 110, 650216 Kunming, P. R. China
3.University of the Chinese Academy of Sciences, Yuquan Road 19#, Shijingshan Block, 100049 Beijing, P. R. China
4.Facultad de Ciencias Astron´omicas y Geof´ısicas, Universidad Nacional de La Plata, 1900 La Plata, Buenos Aires, Argentina
5.Instituto de Astrofisica de La Plata (CCT La plata - CONICET/UNLP), Argentina
6.Department of Theoretical Physics and Astrophysics, Masaryk University, Kotl´aˇrsk´a 2, CZ-611 37 Brno, Czech Republic
7.Sternberg Astronomical Institute, Moscow State University, Universitetskij prospect 13, Moscow 119992, Russia
推荐引用方式
GB/T 7714
Qian SB,Han ZT,Fernández Lajús, E.,et al. Interactions between planets and evolved stars[C]. 见:. Univ Hong Kong, Hong Kong, PEOPLES R CHINA. 2015-12-14.

入库方式: OAI收割

来源:云南天文台

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