Error Analysis of the Light Curve Solution of Contact Binaries Based on the W-D Code | |
Liu L(刘亮)1,2,3,4 | |
刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC |
2021-08 | |
卷号 | 133期号:1026 |
ISSN号 | 0004-6280 |
DOI | 10.1088/1538-3873/ac1ac1 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | We use the idea of repeat measurement to determine the mean value and error of light curve solution parameters of contact binaries. Our simulation is realized by the Monte Carlo algorithm and Wilson-Devinney code. This method can obtain systematic and random errors simultaneously. Within our 48 models, the systematic errors are smaller than the random errors in most cases. According to the numerical calculations, it is found that the relative errors of photometric mass ratios are less than 1% for totally eclipsing contact binaries, while they are generally between 10% and 20% for partly eclipsing ones. The effect of third light on the errors of the photometric solution is also investigated. With a third light, these errors are close to 10% for totally eclipsing contact binaries. Especially, it is better to set the third light to zero in flux if that light is very faint (e.g., less than 1% contribution in luminosity), because such faint third light will bring big errors to the light curve solutions. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星形成与演化 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
资助项目 | National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11773066] ; National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11933008] ; Young Academic and Technology Leaders Project of Yunnan Province[2015HB098] |
WOS关键词 | ADDITIONAL COMPONENTS ; EVOLUTION ; VELOCITY ; SEARCH ; STARS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP PUBLISHING LTD |
WOS记录号 | WOS:000688238100001 |
资助机构 | National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11773066, 11933008] ; Young Academic and Technology Leaders Project of Yunnan Province[2015HB098] |
内容类型 | 期刊论文 |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/24523] |
专题 | 云南天文台_双星与变星研究组 |
通讯作者 | Liu L(刘亮) |
作者单位 | 1.University of Chinese Academy of Sciences, Yuquan Road 19#, Sijingshang Block, Beijing 100049, People's Republic of China 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China; 3.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; 4.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China; LiuL@ynao.ac.cn; |
推荐引用方式 GB/T 7714 | Liu L. Error Analysis of the Light Curve Solution of Contact Binaries Based on the W-D Code[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2021,133(1026). |
APA | Liu L.(2021).Error Analysis of the Light Curve Solution of Contact Binaries Based on the W-D Code.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,133(1026). |
MLA | Liu L."Error Analysis of the Light Curve Solution of Contact Binaries Based on the W-D Code".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 133.1026(2021). |
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