中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Study on the variation of orbital period, quasi-periodic oscillations and negative superhumps in V729 Sgr

文献类型:期刊论文

作者Sun, Qi-Bin4,5; Qian SB(钱声帮)3,4,5; Dong, Ai-Jun4,5; Zhi, Qi-Jun4,5; Han ZT(韩忠涛)3; Liu W(刘伟)3; Chang, Xin2; Liu, Chang4,5; Xiang, Hong-Bin4,5; Peng, Xue-Bing4,5
刊名NEW ASTRONOMY
出版日期2022-05
卷号93
ISSN号1384-1076
关键词Stars Binaries Eclipsing stars Dwarf novae stars Evolution stars Individual V729 sgr
DOI10.1016/j.newast.2021.101751
产权排序第3完成单位
文献子类Article
英文摘要

Based on K2 and our observations of V729 Sgr, the study of the variation of orbital period, quasi-periodic oscillations (QPOs) and negative superhumps are presented. Using all available mid-eclipse times during quiescence, we find that V729 Sgr has a cyclic variation of the orbital period, with periods and amplitudes of 9.64 years and similar to 442.37 s, respectively. Based on the interpret of light travel-time effect, the mass of third body is derived as M(3)sini ' = 0.24(+/- 0.016)M-circle dot. When the third body is coplanar with the central body system, the third body may be a low-mass star. Using the Weighted Wavelet Z-transform (WWZ) method, we find for the first time that V729 Sgr has QPOs with the period of similar to 1030-3370 s. Using WWZ method, we find that V729 Sgr also has negative superhumps in the first quiescence, indicating that the negative superhumps may be permanent in the quiescence of V729 Sgr.

学科主题天文学 ; 恒星与银河系 ; 恒星形成与演化
URL标识查看原文
出版地RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
WOS关键词DWARF NOVA OSCILLATIONS ; EQUATORIAL IRREGULAR VARIABLES ; CATACLYSMIC VARIABLES ; KEPLER OBSERVATIONS ; RAPID OSCILLATIONS ; INSTABILITY ; BINARIES ; SOUTHERN ; MODEL ; DISK
资助项目National Natural Science Foun-dation of China[11933008] ; National Natural Science Foun-dation of China[U1831120] ; National Natural Science Foun-dation of China[U1731238] ; Science and Technology Foundation of Guizhou province[(2019) 1241] ; Science and Technology Foundation of Guizhou province[KY (2020) 003] ; National Key R&D Program of China[2018YFA0404602]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者ELSEVIER
WOS记录号WOS:000820826000003
资助机构National Natural Science Foun-dation of China[11933008, U1831120, U1731238] ; Science and Technology Foundation of Guizhou province[(2019) 1241, KY (2020) 003] ; National Key R&D Program of China[2018YFA0404602]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/25282]  
专题云南天文台_双星与变星研究组
通讯作者Qian SB(钱声帮); Dong, Ai-Jun
作者单位1.Instituto de Astrofísica de La Plata (CCT La plata - CONICET/UNLP), Argentina
2.Department of Physics, Yunnan Normal University, Kunming, 650500, China;
3.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming, 650011, China;
4.Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University, Guiyang, 550001, China;
5.School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550001, China;
推荐引用方式
GB/T 7714
Sun, Qi-Bin,Qian SB,Dong, Ai-Jun,et al. Study on the variation of orbital period, quasi-periodic oscillations and negative superhumps in V729 Sgr[J]. NEW ASTRONOMY,2022,93.
APA Sun, Qi-Bin.,Qian SB.,Dong, Ai-Jun.,Zhi, Qi-Jun.,Han ZT.,...&E, Fernández Lajús,.(2022).Study on the variation of orbital period, quasi-periodic oscillations and negative superhumps in V729 Sgr.NEW ASTRONOMY,93.
MLA Sun, Qi-Bin,et al."Study on the variation of orbital period, quasi-periodic oscillations and negative superhumps in V729 Sgr".NEW ASTRONOMY 93(2022).

入库方式: OAI收割

来源:云南天文台

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