The deep and low-mass-ratio contact binary CSS J022914.4+044340 with a luminous additional companion | |
Liu L(刘亮)1,2,3,4; Li XZ(李旭志)1,2,3,4 | |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2021-08 | |
卷号 | 21期号:7 |
关键词 | binaries : eclipsing binaries : close stars: individuals (CSS J022914.4+044340) stars: evolution |
ISSN号 | 1674-4527 |
DOI | 10.1088/1674-4527/21/7/180 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | The first B-, V-, R-c - and I-c -band light curves of CSS J022914.4+044340 are presented and analyzed. It is found that CSS J022914.4+044340 is a low mass ratio (0.198 +/- 0.005) deep (63.7 +/- 7.9%) contact binary, indicating that it is already at the end evolutionary stage of tidally-locked evolution via magnetized wind. Because of the totally eclipsing character, the photometric solutions are reliable. The temperature and metallicity are determined from the spectroscopic data as T = 5855 +/- 15 K and [Fe/H] = -0.842 +/- 0.031, respectively. Based on the parallax of Gaia EDR3, the physical parameters of CSS J022914.4+044340 are estimated as M-1=1.44(-0.22)(+0.25)M(circle dot) , M-2=0.29(-0.05)(+0.05)M(circle dot) , R-1=1.26(-0.06)(+0.08)R(circle dot) , R-2=0.65(-0.04)(+0.03)R(circle dot) , L-1=1.718(-0.191)(+0.186)L(circle dot) L-2=0.416(-0.050)(+0.039)L(circle dot) . Combining the fraction of light from the third body via the photometric solution (54%), the luminosity of the third body is estimated as 2.705 L (circle dot). The third body may be inferred to be a subgiant. Thus, why the primary component of CSS J022914.4+044340 has higher mass compared to similar systems is explained, as well as why its metallicity is so poor. |
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 | 20A DATUN RD, CHAOYANG, BEIJING, 100012, PEOPLES R CHINA |
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] ; CAS Interdisciplinary Innovation Team ; Young Academic and Technology Leaders Project of Yunnan Province[2015HB098] ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences |
WOS关键词 | URSAE-MAJORIS ; WUMA-TYPE ; LIGHT CURVES ; EVOLUTION ; UMA ; SYSTEMS ; STARS ; COMPONENTS ; CALIBRATIONS ; PARAMETERS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
WOS记录号 | WOS:000691244800001 |
资助机构 | National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC)[11773066, 11933008] ; CAS Interdisciplinary Innovation Team ; Young Academic and Technology Leaders Project of Yunnan Province[2015HB098] ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences |
内容类型 | 期刊论文 |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/24556] |
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, Beijing 100049, China 2.Center for AstronomicalMega-Science, Chinese Academy of Sciences, Beijing 100101, China; 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China; 4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China; |
推荐引用方式 GB/T 7714 | Liu L,Li XZ. The deep and low-mass-ratio contact binary CSS J022914.4+044340 with a luminous additional companion[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2021,21(7). |
APA | Liu L,&Li XZ.(2021).The deep and low-mass-ratio contact binary CSS J022914.4+044340 with a luminous additional companion.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,21(7). |
MLA | Liu L,et al."The deep and low-mass-ratio contact binary CSS J022914.4+044340 with a luminous additional companion".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 21.7(2021). |
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