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Interactions between planets and evolved stars
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; Lajus, F
会议录名称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
2016-08-08
卷号728
期号4
DOI10.1088/1742-6596/728/4/042006
会议录编者/会议主办者Kwok, S; Leung, KC
产权排序第1完成单位
收录类别EI ; CPCI
会议名称11th Pacific Rim Conference on Stellar Astrophysics - Physics and Chemistry of the Late Stages of Stellar Evolution
会议日期2015-12-14
会议地点Univ Hong Kong, Hong Kong, PEOPLES R CHINA
会议赞助商Croucher Fdn; K C Wong Educ Fdn; Univ Hong Kong, Fac Sci
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.

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]
项目资助者Chinese Natural Science Foundation ; Yunnan Natural Science Foundation ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences
语种英语
学科领域天文学 ; 天体物理学
学科门类理学 ; 理学::天文学
文章类型Proceedings Paper
出版者IOP PUBLISHING LTD
出版地DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND
ISSN号1742-6588
URL查看原文
归档日期2016-08-15
WOS记录号WOS:000397958000031
WOS研究方向Astronomy & Astrophysics ; Physics
WOS类目Astronomy & Astrophysics ; Physics, Multidisciplinary
关键词[WOS]Common-envelope Binaries ; Orbital Period Distribution ; Main-sequence Binaries ; White-dwarf ; Eclipsing Binary ; Brown Dwarf ; Hu Aqr ; Cataclysmic Variables ; V2051 Ophiuchi ; Giant Planet
EI入藏号20164102881779
EI主题词White Dwarfs
EI分类号657.2extraterrestrial Physics And Stellar Phenomena
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9798
专题双星与变星研究组
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
第一作者单位中国科学院云南天文台
推荐引用方式
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Qian SB,Han ZT,Fernández Lajús, E.,et al. Interactions between planets and evolved stars[C]//Kwok, S; Leung, KC. DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND:IOP PUBLISHING LTD,2016.
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