The Improved Orbit Solution and Component Masses of bet LMi | |
Wang XL(王晓丽)1,2,3; Xia, Fang4; Fu, Yanning4 | |
发表期刊 | ASTRONOMICAL JOURNAL |
2020-09-01 | |
卷号 | 160期号:3页码:5 |
DOI | 10.3847/1538-3881/aba7bd |
产权排序 | 第2完成单位 |
收录类别 | SCI |
关键词 | Binary stars Fundamental parameters of stars Visual binary stars Spectroscopic binary stars |
摘要 | bet LMi is a double-lined visual binary with an orbital period of similar to 39 yr. Via a simultaneous fitting to both astrometric and radial velocity measurements, we give a complete and improved orbit solution with high precision. Then, the component masses are precisely determined as 2.98 0.10Mand 1.92 0.04Mwith a relative precision of similar to 3%, respectively. The orbital parallax is determined to be 19.6 0.2 mas, which is two times more precise than Hipparcos parallax. With the known apparent magnitudes and magnitude difference of the components, we derive the luminosity of the components as 50.7 1.8Land 9.1 4.1L. The estimated radii of the components are 9.4 0.3Rand 3.7 1.5R. |
资助项目 | National Natural Science Foundation of China[11603072] ; National Natural Science Foundation of China[11727806] ; National Natural Science Foundation of China[11673071] |
项目资助者 | National Natural Science Foundation of China[11603072, 11727806, 11673071] |
语种 | 英语 |
学科领域 | 天文学 ; 恒星与银河系 ; 恒星天文学 |
文章类型 | Article |
出版者 | IOP PUBLISHING LTD |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
ISSN | 0004-6256 |
URL | 查看原文 |
WOS记录号 | WOS:000565725400001 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | ICCD SPECKLE OBSERVATIONS ; BINARY STARS ; INTERFEROMETRIC MEASUREMENTS ; ASTROMETRIC MEASUREMENTS ; VISUAL BINARIES ; KITT-PEAK ; RADIAL-VELOCITIES ; WIYN TELESCOPE ; MERATE ; PISCO |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/23701 |
专题 | 南方基地 中国科学院天体结构与演化重点实验室 |
通讯作者 | Wang XL(王晓丽) |
作者单位 | 1.College of Physics and Electronic Engineering, Qilu Normal University, Jinan, 250200, People's Republic of China 2.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, Kunming 650216, People's Republic of China 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650216, People's Republic of China 4.Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China |
第一作者单位 | 中国科学院云南天文台 |
通讯作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Wang XL,Xia, Fang,Fu, Yanning. The Improved Orbit Solution and Component Masses of bet LMi[J]. ASTRONOMICAL JOURNAL,2020,160(3):5. |
APA | Wang XL,Xia, Fang,&Fu, Yanning.(2020).The Improved Orbit Solution and Component Masses of bet LMi.ASTRONOMICAL JOURNAL,160(3),5. |
MLA | Wang XL,et al."The Improved Orbit Solution and Component Masses of bet LMi".ASTRONOMICAL JOURNAL 160.3(2020):5. |
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文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
The Improved Orbit S(433KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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