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Planets and Brown Dwargs Orbiting Evolved Binaries
Qian SB(钱声帮)1,2,3; Zhu LY(朱俐颖)1,2,3; Liao WP(廖文萍)1,2; M. Zejda4; Z. Mikulášek4; E. Fernández Lajús5,6; S. Zola7,8; Zhou X(周肖)1,2,3; Han ZT(韩忠涛)1,2,3; Qian, SB (reprint author), Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
会议录名称Astronomical Society of the Pacific (ASP) Conference Series - LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES
2015-07
卷号496
页码388-393
产权排序第1完成单位
收录类别CPCI
会议名称Conference on Living Together: Planets, Host Stars and Binaries
会议日期2014-09-08
会议地点Litomysl, CZECH REPUBLIC
摘要Searches for planets and brown dwarf companions to evolved close binary stars (e.g., detached WD+dM binaries, sdB-type eclipsing binaries, magnetic CVs, and X-ray binaries) can provide insight into the formation and ultimate fate of circumbinary planets and brown dwarfs, as well as shed light on the late evolution of binary stars. The eclipse timing method has most successfully been applied to detect extrasolar planets around binary stars evolved beyond the first red-giant branch. We have monitored different types of evolved eclipsing binaries using this method since 2006. In this paper we review some observational results of circumbinary planets and brown dwarfs orbiting evolved binaries, especially those orbiting sdB-type eclipsing binaries. The fate of the Earth in our solar system is discussed by a comparison of the observational properties of the close-in substellar objects orbiting sdB-type binaries with those of planets in our solar system.
语种英语
文章类型Proceedings Paper
出版者ASTRONOMICAL SOC PACIFIC
出版地390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
ISBN号978-1-58381-877-0; 978-1-58381-876-3
URL查看原文
归档日期2015-08-12
WOS记录号WOS:000369467900092
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics ; Astronomy & Astrophysics
关键词[WOS]ECLIPSING BINARY ; CIRCUMBINARY PLANET ; COMPANION ; SYSTEM ; STARS ; VIR
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9667
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Qian, SB (reprint author), Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
作者单位1.Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650011 Kunming, P.R. China;
2.Key laboratory of the structure and evolution celestial bodies, Chinese Academy of Sciences, P. O. Box 110, 650011 Kunming, P. R. China
3.University of the Chinese Academy of Sciences, Yuquan Road 19#, Sijingshang Block, 100049 Beijing, P. R. China
4.Department of Theoretical Physics and Astrophysics, Masaryk University, Kotláˇrská 2, CZ-611 37 Brno, Czech Republic
5.Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, 1900 La Plata, Buenos Aires, Argentina
6.Instituto de Astrofisica de La Plata (CCT La Plata - CONICET/UNLP), Argentina
7.Astronomical Observatory, Jagiellonian University, ul. Orla 171, 30-244 Kraków, Poland
8.Mt. Suhora Observatory, Pedagogical University, ul. Podchorazych 2, 30-084 Kraków, Poland
推荐引用方式
GB/T 7714
Qian SB,Zhu LY,Liao WP,et al. Planets and Brown Dwargs Orbiting Evolved Binaries[C]. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2015:388-393.
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