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Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-resolution Survey

文献类型：期刊论文

作者Guo SF(郭素芬)1,2,3,4; Kovalev, Mikhail2,3,4; Li J(李蛟)2,3,4; Lü, Guoliang1; Jia S(贾石)2,3,4; Li ZW(李振威)2,3,4; Li JD(李江丹)2,3,4; Xiong JP(熊建萍)2,3,4; Yang, Mingkuan5; He TY(何同禹)4,6
刊名ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
出版日期2025-06-01
卷号278期号:2
ISSN号0067-0049
DOI10.3847/1538-4365/adced1
产权排序第2完成单位
文献子类Article
英文摘要The period, mass ratio, eccentricity, and other orbital parameters are fundamental for investigating binary star evolution. However, the number of binaries with known orbital parameters remains limited. Utilizing the LAMOST medium-resolution spectroscopic survey, we derived orbital solutions for 665 SB 2 binaries by fitting the radial velocities of 1119 SB 2 systems with at least six observations, employing a modified version of The Joker optimized for SB 2 binaries. To ensure the reliability of the results, four selection criteria were applied: reduced chi-square, normalized mean absolute error, maximum phase gap, and radial velocity distribution metric. After applying these criteria, 665 reliable orbits were retained. Comparison with Kepler, TESS, and Zwicky Transient Facility light-curve data shows excellent agreement, with discrepancies in some cases attributed to shorter pulsation periods observed in light curves. Additionally, good consistency is found between our periods and those of SB 1 systems in Gaia data. These orbital solutions contribute to understanding binary star evolution and the statistical properties of binary populations.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词ECLIPSING BINARIES ; DATA RELEASE ; APOGEE DR16 ; STELLAR ; STARS ; EVOLUTION ; CANDIDATES ; ASTROPY ; MASS ; CLASSIFICATION
资助项目MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12288102]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12125303]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12090040/3]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12463011]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12403040]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12003025]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12373038]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[U2031204]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12163005]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12433009]; MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12473034]; National Natural Science Foundation of China[2021YFA1600400/1]; National Natural Science Foundation of China[2021YFA1600403]; National Key R&D Program of China[XDB1160201]; National Key R&D Program of China[XDB1160000]; Strategic Priority Research Program of the Chinese Academy of Sciences[202305AB350003]; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202302AN360001]; Yunnan Key Laboratory of Supernova Research[2024D01C230]; Natural Science Foundation of Xinjiang[XJEDU2022P003]; Scientific Research Program of the Higher Education Institution of Xinjiang[202401BC070007]; Scientific Research Program of the Higher Education Institution of Xinjiang[202401AT070139]; Scientific Research Program of the Higher Education Institution of Xinjiang[202201BC070003]; Scientific Research Program of the Higher Education Institution of Xinjiang[202301AT070314]; Yunnan Fundamental Research Projects[ZDBS-LY-7005]; Key Research Program of Frontier Sciences of CAS[202401CF070035]; Yunnan Fundamental Research Projects (YFRP); Young Talent Project of Yunnan Revitalization Talent Support Program; Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST); National Development and Reform Commission; Chinese Academy of Sciences
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001508413100001
出版者IOP Publishing Ltd
资助机构MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809[12288102, 12125303, 12090040/3, 12463011, 12403040, 12003025, 12373038, U2031204, 12163005, 12433009, 12473034] ; National Natural Science Foundation of China[2021YFA1600400/1, 2021YFA1600403] ; National Key R&D Program of China[XDB1160201, XDB1160000] ; Strategic Priority Research Program of the Chinese Academy of Sciences[202305AB350003] ; Yunnan Revitalization Talent Support Program-Science and Technology Champion Project[202302AN360001] ; Yunnan Key Laboratory of Supernova Research[2024D01C230] ; Natural Science Foundation of Xinjiang[XJEDU2022P003] ; Scientific Research Program of the Higher Education Institution of Xinjiang[202401BC070007, 202401AT070139, 202201BC070003, 202301AT070314] ; Yunnan Fundamental Research Projects[ZDBS-LY-7005] ; Key Research Program of Frontier Sciences of CAS[202401CF070035] ; Yunnan Fundamental Research Projects (YFRP) ; Young Talent Project of Yunnan Revitalization Talent Support Program ; Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, LAMOST) ; National Development and Reform Commission ; Chinese Academy of Sciences
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28370]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
通讯作者Li J(李蛟)
作者单位1.School of Physical Science and Technology, Xinjiang University, Urumqi 830046, People's Republic of China;
2.Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People's Republic of China; lijiao@ynao.ac.cn, zhanwenhan@ynao.ac.cn;
3.Key Laboratory for the Structure and Evolution of Celestial Objects, CAS, Kunming 650216, People's Republic of China;
4.International Centre of Supernovae (ICESUN), Yunnan Key Laboratory of Supernova Research, Yunnan Observatories, Chinese Academy of Sciences (CAS), Kunming 650216, People's Republic of China;
5.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China;
6.College of Physics Science and Technology, Hebei University, Baoding 071002, People's Republic of China
推荐引用方式
GB/T 7714		 Guo SF,Kovalev, Mikhail,Li J,et al. Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-resolution Survey[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2025,278(2).
APA 郭素芬.,Kovalev, Mikhail.,李蛟.,Lü, Guoliang.,贾石.,...&韩占文.(2025).Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-resolution Survey.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,278(2).
MLA 郭素芬,et al."Orbital Parameters of 665 Double-lined Spectroscopic Binaries in the LAMOST Medium-resolution Survey".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 278.2(2025).

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