Interactions between planets and evolved stars

doi:10.1088/1742-6596/728/4/042006

	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, Zejda 6; Li LJ(李临甲)1,2 ; Voloshina, Irina 7; Liu L(刘亮)1,2,3 ; He JJ(何家佳)1,2
	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
DOI	10.1088/1742-6596/728/4/042006
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
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
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
会议录出版者	IOP PUBLISHING LTD
会议录出版地	DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND
文献子类	Proceedings Paper
学科主题	天文学 ; 天体物理学
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
内容类型	会议论文
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.