中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Long Photometric Cycles in Double-periodic Variables from Nodal Precession of a Tilted Accretion Disk

文献类型:期刊论文

作者Jiao CL(焦承亮)1,4,5; Zhao EG(赵二刚)1,4; Zhu LY(朱俐颖)1,3,4; Matekov, Azizbek2,3,4
刊名ASTROPHYSICAL JOURNAL
出版日期2026-03-20
卷号1000期号:1
ISSN号0004-637X
DOI10.3847/1538-4357/ae4b30
产权排序第1完成单位
文献子类Article
英文摘要We investigate whether the long photometric cycles observed in double-periodic variables (DPVs) can arise from nodal precession of a tilted accretion disk driven by the tidal torque of the companion. Within a simple analytical framework, we derive testable relations linking the long-to-orbital period ratio to the binary mass ratio, the normalized disk size, and the disk tilt angle beta, which itself can be inferred from the long-cycle amplitude, orbital inclination i, and disk luminosity fraction. The model naturally reproduces the two observed long-cycle light-curve morphologies-sinusoidal and double hump-distinguished by the geometric criterion i + beta <= 90 degrees versus i + beta > 90 degrees. Applying these relations to a sample of DPVs, we find that the inferred disk sizes are physically reasonable and consistent with independent light-curve modeling for a nonnegligible subset of systems. Our results show that tidal nodal precession represents a viable and potentially important contributor to the long-period variability of DPVs and provide a quantitative framework for future observational and theoretical studies.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词HD 170582 ; BINARY ; PARAMETERS ; STELLAR ; MODEL ; SPECTROSCOPY ; VARIABILITY ; STARS
资助项目(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic) divided by Natural Science Foundation of Yunnan Province (Yunnan Natural Science Foundation)[202401AS070046]; Bureau of International Cooperation, Chinese Academy of Sciences[020GJHZ2023030GC]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001717971000001
出版者IOP Publishing Ltd
资助机构(sic)(sic)(sic)(sic)(sic)(sic)(sic)(sic) divided by Natural Science Foundation of Yunnan Province (Yunnan Natural Science Foundation)[202401AS070046] ; Bureau of International Cooperation, Chinese Academy of Sciences[020GJHZ2023030GC]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/29063]  
专题云南天文台_双星与变星研究组
通讯作者Jiao CL(焦承亮)
作者单位1.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People’s Republic of China;
2.Ulugh Beg Astronomical Institute, Uzbekistan Academy of Sciences, 33 Astronomicheskaya str., Tashkent, 100052, Uzbekistan
3.University of Chinese Academy of Sciences, No. 1 Yanqihu East Road, Huairou District, 101408, Beijing, People’s Republic of China;
4.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People’s Republic of China; jiaocl@ynao.ac.cn, zergang@ynao.ac.cn;
5.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, People’s Republic of China;
推荐引用方式
GB/T 7714
Jiao CL,Zhao EG,Zhu LY,et al. Long Photometric Cycles in Double-periodic Variables from Nodal Precession of a Tilted Accretion Disk[J]. ASTROPHYSICAL JOURNAL,2026,1000(1).
APA 焦承亮,赵二刚,朱俐颖,&Matekov, Azizbek.(2026).Long Photometric Cycles in Double-periodic Variables from Nodal Precession of a Tilted Accretion Disk.ASTROPHYSICAL JOURNAL,1000(1).
MLA 焦承亮,et al."Long Photometric Cycles in Double-periodic Variables from Nodal Precession of a Tilted Accretion Disk".ASTROPHYSICAL JOURNAL 1000.1(2026).

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来源:云南天文台

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