The first multi-color photometric study of the short-period contact eclipsing binary GK Aqr
文献类型:期刊论文
作者 | Zhang, LY1,2![]() ![]() ![]() |
刊名 | NEW ASTRONOMY
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出版日期 | 2015-07 |
卷号 | 38页码:50-54 |
关键词 | Stars: binaries: eclipsing Stars: period variation Stars: individual GK Aqr |
ISSN号 | 1384-1076 |
产权排序 | 第四完成单位 |
通讯作者 | Zhang, LY (reprint author), Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China. |
英文摘要 | We made the first VRI CCD light curves of the short-period contact eclipsing binary GM Aqr, which was observed on October 5 and 8, 2013 at Xinglong station of National Astronomical Observatories, China. The ephemeris of GK Aqr was calculated based on our two newly obtained minima and the minima that other observers obtained previously. We discovered that the orbital period of GK Aqr exhibits an increasing trend of P = 2.8(0.1) x 10(-7) days/year by means of fitting the O-C values of the minima. This phenomenon might be explained by mass transfer from the primary (less massive) component to the secondary (more massive) one. With the updated Wilson & Devinney program, we obtained the photometric orbital parameters for the first time. Using our parameters, we also successfully explained the light curve obtained from the All Sky Automated Survey data. In the end, we concluded that GK Aqr is a near contact binary with a low contact factor of 5.2%. As the mass transfer continues, GK Aqr could become a contact system and evolve into an over-contact system. (C) 2015 Elsevier B.V. All rights reserved. |
WOS标题词 | Science & Technology ; Physical Sciences |
学科主题 | Astronomy & Astrophysics |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | VARIABLE-STARS ; LIGHT CURVES ; CATALOG |
收录类别 | SCI |
原文出处 | http://www.sciencedirect.com/science/article/pii/S1384107615000160 |
语种 | 英语 |
WOS记录号 | WOS:000351979500006 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5463] ![]() |
专题 | 云南天文台_丽江天文观测站(南方基地) 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.College of Science/Department of Physics & NAOC-GZU-Sponsored Center for Astronomy Research, Guizhou University, Guiyang 550025, PR China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, PR China 3.Dept. of Physics and Astronomy, Butler University, Indianapolis, IN 46208, USA 4.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, PR China 5.School of Mathematics Science, Liaocheng University, Liaocheng 252059, PR China |
推荐引用方式 GB/T 7714 | Zhang, LY,Pi, QF,Han, XML,et al. The first multi-color photometric study of the short-period contact eclipsing binary GK Aqr[J]. NEW ASTRONOMY,2015,38:50-54. |
APA | Zhang, LY.,Pi, QF.,Han, XML.,Li, TA.,Zhang XL.,...&Wang, S.(2015).The first multi-color photometric study of the short-period contact eclipsing binary GK Aqr.NEW ASTRONOMY,38,50-54. |
MLA | Zhang, LY,et al."The first multi-color photometric study of the short-period contact eclipsing binary GK Aqr".NEW ASTRONOMY 38(2015):50-54. |
入库方式: OAI收割
来源:云南天文台
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