YNAO OpenIR  > 双星与变星研究组
Circumbinary Planets Orbiting Around Post Common Envelope Binaries
Zhu LY(朱俐颖)1,2,3; Qian SB(钱声帮)1,2,3; Liao WP(廖文萍)1,2; E. Fernandez Laj ´ us4,5; B. Soonthornthum6; Zhao EG(赵二刚)1,2,3; Liu L(刘亮)1,2,3
Source PublicationPublications of The Korean Astronomical Society - Proceedings of Asian-Pacific Regional IAU Meeting(APRIM2014)
2015-09
Volume30
Issue2
Pages289-292
DOI10.5303/PKAS.2015.30.2.289
Contribution Rank第1完成单位
Indexed By其他
Conference Name12th Asia-Pacific Regional IAU Meeting
Conference Date2014-08-18
Conference PlaceDOC, Daejeon, Korea
KeywordBinaries:Close Binaries: Eclipsing Planetary System
Abstract

Most of the stars in the Galaxy are in binary systems. Binaries should be possible as the hosting stars of planets. Searching for planetary companions to binaries, especially evolved close binary stars, can provide insight into the formation and the ultimate fate of circumbinary planets and shed light on the late evolution of binary stars. In order to do this, we have chosen some post common envelope binaries including sdB-type eclipsing binaries and detached WD+dM eclipsing binaries as our targets and monitored them for several years. In this paper, we will present some of our new observations and results for three targets, NSVS 07826147, NSVS14256825 and RR Cae.

Funding ProjectChinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[11325315] ; Yunnan Natural Science Foundation[2013FB084] ; young academic leaders project of Yunnan Province
Funding OrganizationChinese Natural Science Foundation ; Yunnan Natural Science Foundation ; young academic leaders project of Yunnan Province
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
PublisherThe Korean Astronomical Society
Publication PlaceKorea
ISSN1225-1534
URL查看原文
Archive Date2015-11-25
Citation statistics
Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9677
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 AuthorZhu LY(朱俐颖)
Affiliation1.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, P.R. China
2.Key Laboratory for the Structure and Evolution of Celestial Bodies, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, P. R. China
3.Physical Sciences Department, Graduate University of the Chinese Academy of Sciences, Yuquan Road 19, Sijingshang Block, 100049 Beijing, China
4.Facultad de Ciencias Astron´omicasy 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.National Astronomical Research Institute of Thailand, 191 Siriphanich Bidg.2nd Fl. Huay Kaew Rd. Suthep District, Muang, Chiang Mai 50200, Thailand
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhu LY,Qian SB,Liao WP,et al. Circumbinary Planets Orbiting Around Post Common Envelope Binaries[C]. Korea:The Korean Astronomical Society,2015:289-292.
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