Institutional Repository of Optical Astronomy Research Laboratory
| KIC 10417986: Spectroscopic Confirmation of the Nature of the Binary System with a delta Scuti Component | |
Feng, Guo-Jie1,2 ; Esamdin, Ali1,2; Fu, Jian-Ning3; Niu, Hu-Biao1; Zong, Peng3; Yang, Tao-Zhi4; Ma, Shu-Guo1,2; Xu, Jing1; Bai, Chun-Hai1; Wang, Yong1; Sun, Wei-Chao1; Wang, Xin-Liang1
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| 2022-10-01 | |
| Source Publication | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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| ISSN | 1674-4527 |
| Volume | 22Issue:10Pages:105005 |
| Contribution Rank | 1 |
| Abstract | KIC 10417986 is a short orbital period (0.0737 day) ellipsoidal variable star with a delta Sct and gamma Dor hybrid pulsation component discovered by Kepler. The ground-based spectroscopic observations were carried out in the winters of 2020 and 2021 to investigate the binary nature of this star. We derive the orbital parameters using the rvfit code with a result of K-1 = 29.7 +/- 1.5 km s(-1), gamma = -18.7 +/- 1.7 km s(-1), and confirm an orbital period of 0.84495 day instead of the result given by Kepler. The atmospheric parameters of the primary are determined by the synthetic spectral fitting technique with the estimated values of T-eff = 7411 +/- 187 K, log g = 4.2 +/- 0.3 dex, [M/H] = 0.08 +/- 0.09 dex and vsini = 52 +/- 11 km s(-1). KIC 10417986 is a circular orbit binary system. From the single-lined nature and mass function of the star, the derived orbital inclination is 26 degrees +/- 6 degrees, and the mass of the secondary is 0.52(-0.09)(+0.18) M-circle dot, which should be a late-K to early-M type star. Fourteen frequencies are extracted from Kepler light curves, of which six independent frequencies in the high-frequency region are identified as the p-mode pulsations of delta Sct star, and one independent frequency in the low-frequency region (f(2) = 1.3033 cd(-1)) is probably the rotational frequency due to the starspots rather than the ellipsoidal effect. |
| Keyword | techniques: spectroscopic (stars:) binaries: spectroscopic stars: individual (KIC 10417986) stars: oscillations (including pulsations) stars: variables: delta Scuti (stars:) starspots |
| DOI | 10.1088/1674-4527/ac8b5c |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | COMBINATION FREQUENCIES ; DIFFERENTIAL ROTATION ; ECLIPSING BINARY ; STARS ; KEPLER ; PERIOD ; VARIABILITY ; PULSATIONS ; AMPLITUDE ; SPECTRA |
| Funding Project | National Natural Science Foundation of China (NSFC)[11403088] ; National Natural Science Foundation of China (NSFC)[11873081] ; National Natural Science Foundation of China (NSFC)[U2031209] ; National Natural Science Foundation of China (NSFC)[11833002] ; National Natural Science Foundation of China (NSFC)[12090040] ; National Natural Science Foundation of China (NSFC)[12090042] ; National Natural Science Foundation of China (NSFC)[12003020] ; Nanshan 1.2 m telescope of XinjiangAstronomical Observatory, Chinese Academy of Sciences ; NASA Science Mission directorate ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000859105600001 |
| Publisher | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
| Funding Organization | National Natural Science Foundation of China (NSFC) ; Nanshan 1.2 m telescope of XinjiangAstronomical Observatory, Chinese Academy of Sciences ; NASA Science Mission directorate ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/4891 |
| Collection | 光学天文与技术应用研究室 |
| Corresponding Author | Esamdin, Ali |
| Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 4.Xi An Jiao Tong Univ, Minist Educ, Key Lab Nonequilibrium Synth & Modulat Condensed, Xian 710049, Peoples R China |
| First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Feng, Guo-Jie,Esamdin, Ali,Fu, Jian-Ning,et al. KIC 10417986: Spectroscopic Confirmation of the Nature of the Binary System with a delta Scuti Component[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2022,22(10):105005. |
| APA | Feng, Guo-Jie.,Esamdin, Ali.,Fu, Jian-Ning.,Niu, Hu-Biao.,Zong, Peng.,...&Wang, Xin-Liang.(2022).KIC 10417986: Spectroscopic Confirmation of the Nature of the Binary System with a delta Scuti Component.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,22(10),105005. |
| MLA | Feng, Guo-Jie,et al."KIC 10417986: Spectroscopic Confirmation of the Nature of the Binary System with a delta Scuti Component".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 22.10(2022):105005. |
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| Feng-2022-KIC 104179（3232KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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