Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries

doi:10.3847/1538-4365/ad226a

CORC > 云南天文台 > 中国科学院云南天文台 > 丽江天文观测站（南方基地）

	Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries
	Li, Xu-Zhi 1,5; Zhu, Qing-Feng 1,2,5; Ding X(丁旭)4,6,7; Xu, Xiao-Hui 1,5; Zheng, Hang 1,5; Qiu, Jin-Sheng 1,5; Liu MC(刘明超)3,7
刊名	ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
	2024-03-01
卷号	271 期号:1
ISSN号	0067-0049
DOI	10.3847/1538-4365/ad226a
产权排序	第4完成单位
文献子类	Article
英文摘要	Starting from more than 11,200 short-period (less than 0.5 days) EW-type eclipsing binary candidates with the All-Sky Automated Survey for Supernovae V-band light curves, we use the Markov Chain Monte Carlo algorithm and neural networks to obtain the mass ratio (q), orbital inclination (incl), fill-out factor (f), and temperature ratio (T s /T p ). After crossmatching with the Gaia DR3 database, the final sample contains parameters of 2399 A-type and 8712 W-type contact binaries (CBs). We present the distributions of parameters of these 11,111 short-period CBs. The mass ratio (q) and fill-out factor (f) are found to obey log-normal distributions, and the remaining parameters obey normal distributions. There is a significant period-temperature correlation of these CBs. Additionally, the temperature ratio (T s /T p ) tends to increase as the orbital period decreases for W-type CBs. There is no significant correlation between them for A-type CBs. The mass ratio and fill-out factor (q-f) diagram suggest there is no significant correlation between these two parameters. A clear correlation exists between the mass ratio and radius ratio. The radius ratio increases with the mass ratio. Moreover, the deep fill-out CBs tend to fall on the upper boundary of the q-R s /R p distribution, while the shallow fill-out CBs fall on the lower boundary.
学科主题	天文学
URL标识	查看原文
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
资助项目	MOST divided by National Key Research and Development Program of China (NKPs)https://doi.org/10.13039/501100012166[2023YFA1608100]; National Key Research and Development Program of China[2308085QA35]; Anhui Provincial Natural Science Foundation[XDB 41000000]; Strategic Priority Research Program of the Chinese Academy of Sciences[2021M703099]; China Postdoctoral Science Foundation; Fundamental Research Funds for the Central Universities
WOS关键词	VARIABLE-STARS ; LIGHT CURVES ; EVOLUTIONARY STATUS ; COBITOM PROJECT ; OGLE COLLECTION ; CLOSE BINARIES ; CATALOG ; I. ; VARIABILITY ; SYSTEMS
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP Publishing Ltd
WOS记录号	WOS:001179739700001
资助机构	MOST divided by National Key Research and Development Program of China (NKPs)https://doi.org/10.13039/501100012166[2023YFA1608100] ; National Key Research and Development Program of China[2308085QA35] ; Anhui Provincial Natural Science Foundation[XDB 41000000] ; Strategic Priority Research Program of the Chinese Academy of Sciences[2021M703099] ; China Postdoctoral Science Foundation ; Fundamental Research Funds for the Central Universities
内容类型	期刊论文
版本	出版稿
源URL	[http://ir.ynao.ac.cn/handle/114a53/26557]
专题	云南天文台_丽江天文观测站（南方基地）
作者单位	1.School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei, 230026, People's Republic of China; 2.Deep Space Exploration Laboratory, Hefei 230088, People's Republic of China; 3.University of the Chinese Academy of Sciences, Yuquan Road 19, Shijingshan Block, Beijing, 100049, People's Republic of China 4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China; 5.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, 230026, People's Republic of China; lixuzhi@ustc.edu.cn, zhuqf@ustc.edu.cn; 6.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P.O. Box 110, 650216 Kunming, People's Republic of China; 7.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, Yunnan, People's Republic of China; dingxu@ynao.ac.cn;
推荐引用方式 GB/T 7714	Li, Xu-Zhi,Zhu, Qing-Feng,Ding X,et al. Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2024,271(1).
APA	Li, Xu-Zhi.,Zhu, Qing-Feng.,丁旭.,Xu, Xiao-Hui.,Zheng, Hang.,...&刘明超.(2024).Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,271(1).
MLA	Li, Xu-Zhi,et al."Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 271.1(2024).