中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Photometric Properties and Stellar Parameters of the Rapidly Rotating Magnetic Early-B Star HD 345439

文献类型:期刊论文

作者Shen, Dong-Xiang2; Liu, Jin-Zhong1; Zhu, Chun-Hua2; Lu, Guo-Liang2; Zhang, Yu1; Lu, Cheng-Long1; Wang, Hao-Zhi1; Li, Lei2; Lu, Xi-Zhen2; Yu, Jin-Long2
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2023
卷号23期号:1页码:14
关键词stars: chemically peculiar stars: early-type stars: fundamental parameters stars: magnetic field
ISSN号1674-4527
DOI10.1088/1674-4527/ac9f07
通讯作者Liu, Jin-Zhong(liujinzh@xao.ac.cn)
英文摘要We first present the multicolor photometry results of the rapidly rotating magnetic star HD 345439 using the Nanshan One-meter Wide-field Telescope. From the photometric observations, we derive a rotational period of 0.7699 +/- 0.0014 day. The light curves of HD 345439 are dominated by the double asymmetric S-wave feature that arises from the magnetic clouds. Pulsating behaviors are not observed in Sector 41 of the Transiting Exoplanet Survey Satellite. No evidence is found of the occurrence of centrifugal breakout events neither in the residual flux nor in the systematic variations at the extremum of the light curve. Based on the hypothesis of the Rigidly Rotating Magnetosphere model, we restrict the magnetic obliquity angle beta and the rotational inclination angle i so that they satisfy the approximate relation beta + i asymptotic to 105 degrees. The color excess, extinction, and luminosity are determined to be E ((B-V)) = 0.745 +/- 0.016 mag, A(V) = 2.31 +/- 0.05 mag, and log(L/L-circle dot)=3.82 +/- 0.1 dex, respectively. Furthermore, we derive the effective temperature as T-eff = 22 +/- 1 kK and the surface gravity as log g = 4.00 +/- 0.22. The mass M=7.24(-1.24)(+1.75)M(circle dot), radius R = 4.44(-1.93)(+2.68) R-circle dot=-tau(age) = 23.62(-21.97)(+4.24) Myr are estimated from the Hertzsprung-Russell diagram.
WOS关键词SPECTRAL VARIABILITY ; ATMOSPHERIC PARAMETERS ; MAGNETOSPHERE MODEL ; FIELD MEASUREMENTS ; VARIABLE-STARS ; MASSIVE STARS ; ALPHA-BRIGHT ; DISCOVERY ; EMISSION ; CLUSTER
资助项目Natural Science Foundation of Xinjiang[2021D01C075] ; National Natural Science Foundation of China[U2031204] ; National Natural Science Foundation of China[12163005] ; National Natural Science Foundation of China[11863005] ; China Manned Space Project[CMS-CSST-2021-A08] ; China Manned Space Project[CMS-CSST-2021-A10] ; National Key R&D Program of China[2022YFE0126200] ; National Development and Reform Commission ; NASA[NAS 526555]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000905390700001
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
资助机构Natural Science Foundation of Xinjiang ; National Natural Science Foundation of China ; China Manned Space Project ; National Key R&D Program of China ; National Development and Reform Commission ; NASA
源URL[http://ir.xao.ac.cn/handle/45760611-7/5035]  
专题新疆天文台_光学天文与技术应用研究室
光学天文与技术应用研究室_利用南山1米大视场望远镜(NOWT)观测数据的文章
通讯作者Liu, Jin-Zhong
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, Natl Astron Observ, Urumqi 830000, Peoples R China
2.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Peoples R China
推荐引用方式
GB/T 7714
Shen, Dong-Xiang,Liu, Jin-Zhong,Zhu, Chun-Hua,et al. Photometric Properties and Stellar Parameters of the Rapidly Rotating Magnetic Early-B Star HD 345439[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2023,23(1):14.
APA Shen, Dong-Xiang.,Liu, Jin-Zhong.,Zhu, Chun-Hua.,Lu, Guo-Liang.,Zhang, Yu.,...&Rustem, Abdurepqet.(2023).Photometric Properties and Stellar Parameters of the Rapidly Rotating Magnetic Early-B Star HD 345439.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,23(1),14.
MLA Shen, Dong-Xiang,et al."Photometric Properties and Stellar Parameters of the Rapidly Rotating Magnetic Early-B Star HD 345439".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 23.1(2023):14.

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