NSVS 01286630: a detached binary with a close-in companion
文献类型:期刊论文
作者 | Zhang B(张斌)1,2,3; Qian SB(钱声帮)1,2,3; Liao WP(廖文萍)1,2,3; Zhu LY(朱俐颖)1,2,3; Dong, Ai-Jun4; Zhi, Qi-Jun4 |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
出版日期 | 2018-08-01 |
卷号 | 18期号:9页码:10 |
ISSN号 | 1674-4527 |
关键词 | stars: binaries: close stars: binaries: eclipsing stars: individual (NSVS 01286630) |
DOI | 10.1088/1674-4527/18/9/116 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | New photometric observations of NSVS 01286630 were performed and two sets of fourcolor (B, V, R-c, I-c) light curves (LCs) were obtained. Using the 2013 version of the Wilson-Devinney (W-D) code, we analyzed these data. The photometric solutions reveal that NSVS 01286630 is an active detached eclipsing binary (EB) with a high orbital inclination (nearly 90 degrees). Remarkably, the temperature of the primary component (the hotter star) is higher than the secondary one, but the value of mass ratio q(M-2/M-1) for NSVS 0128663 is more than 1, which can be explained in that the surface of the secondary component of NSVS 01286630 is covered with big cool starspots. Based on our new CCD mid-eclipse times and the data published until now, variations in the mid-eclipse times were reanalyzed in detail using a weighted least-squares method. It is discovered that the (O - C) diagram of the system shows a cyclic oscillation with a period of 3.61 yr and an amplitude of 0.001 d. The cyclic variation may be caused by the light-travel time effect (LTTE) due to the presence of a third companion, whose mass we calculated as M-3 sin(i(3)) = 0. 11M(circle dot). The third body may affect the orbital evolution of the central binary system by transferring angular momentum. |
学科主题 | 天文学 |
URL标识 | 查看原文 |
出版地 | CHIN ACAD SCIENCES, 20A DATUN RD, CHAOYANG, BEIJING, 100012, PEOPLES R CHINA |
WOS关键词 | LOW-MASS STARS ; ORBITAL PERIOD MODULATION ; SKY-VARIABILITY-SURVEY ; ECLIPSING BINARY ; MAGNETIC ACTIVITY ; LIGHT CURVES ; RT LACERTAE ; EVOLUTION ; SYSTEMS ; CYCLES |
资助项目 | National Natural Science Foundation of China[11573063] ; National Natural Science Foundation of China[11611530685] ; Key Science Foundation of Yunnan Province[2017FA001] ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences |
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:000445688500012 |
资助机构 | National Natural Science Foundation of China[11573063, 11611530685] ; Key Science Foundation of Yunnan Province[2017FA001] ; Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences |
源URL | [http://ir.ynao.ac.cn/handle/114a53/17910] |
专题 | 云南天文台_双星与变星研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Zhang B(张斌) |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China 2.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China 3.University of Chinese Academy of Sciences, Beijing 100049, China 4.School of Physics and Electronic Science, Guizhou Normal University, Guiyang 550001, China |
推荐引用方式 GB/T 7714 | Zhang B,Qian SB,Liao WP,et al. NSVS 01286630: a detached binary with a close-in companion[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2018,18(9):10. |
APA | Zhang B,Qian SB,Liao WP,Zhu LY,Dong, Ai-Jun,&Zhi, Qi-Jun.(2018).NSVS 01286630: a detached binary with a close-in companion.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,18(9),10. |
MLA | Zhang B,et al."NSVS 01286630: a detached binary with a close-in companion".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 18.9(2018):10. |
入库方式: OAI收割
来源:云南天文台
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