YNAO OpenIR  > 双星与变星研究组
Planets and Brown Dwarfs 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; Zejda, M4; Mikulasek, Z4; Lajus, EF5,6; Zola, S7,8; Zhou X(周肖)1,2,3; Han ZT(韩忠涛)1,2,3
Source PublicationAstronomical Society of the Pacific (ASP) Conference Series - LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES
2015-07
Volume496
Pages388-393
Author of SourceRucinski, SM; Torres, G; Zejda, M
Contribution Rank第1完成单位
Indexed ByCPCI
Conference NameConference on Living Together: Planets, Host Stars and Binaries
Conference Date2014-09-08
Conference PlaceLitomysl, CZECH REPUBLIC
Conference SponsorSci Org Comm
Abstract

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.

Funding ProjectChinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[11325315] ; Ministry of Education of the Czech Republic[LG12001]
Funding OrganizationChinese Natural Science Foundation ; Ministry of Education of the Czech Republic
Language英语
Subject Area天文学 ; 天体物理学 ; 恒星与银河系
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeProceedings Paper
PublisherASTRONOMICAL SOC PACIFIC
Publication Place390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
ISBN978-1-58381-877-0; 978-1-58381-876-3
URL查看原文
WOS IDWOS:000369467900092
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordEclipsing Binary ; Circumbinary Planet ; Companion ; System ; Stars ; Vir
Citation statistics
Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9703
Collection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
Corresponding AuthorQian SB(钱声帮)
Affiliation1.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, ChineseAcademy 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 LaPlata, 1900 La Plata, Buenos Aires, Argentina
6.Instituto de Astrofisica de La Plata (CCT La Plata - CONICET/UNLP),Argentina
7.7Astronomical Observatory, Jagiellonian University, ul. Orla 171, 30-244Kraków, Poland
8.Mt. Suhora Observatory, Pedagogical University, ul. Podchorazych 2, 30-084 Kraków, Poland
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Qian SB,Zhu LY,Liao WP,et al. Planets and Brown Dwarfs Orbiting Evolved Binaries[C]//Rucinski, SM; Torres, G; Zejda, M. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2015:388-393.
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