中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A Preliminary Photometric Study of the HW Vir-like Binary NSVS14256825

文献类型:会议论文

作者Zhu LY(朱俐颖); Qian SB(钱声帮); Liu L(刘亮); Liao WP(廖文萍); He JJ(何家佳); Li LJ(李临甲); Zhao EG(赵二刚); Dai ZB(戴智斌); Zhang J(张嘉); Li K(李凯)
出版日期2012
会议名称9th Pacific Rim Conference on Stellar Astrophysics
会议日期2011-04-14
会议地点Lijiang, PEOPLES R CHINA
卷号451
页码155-158
通讯作者Zhu, LY (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, POB 110, Kunming 650011, Peoples R China.
英文摘要HW Vir-like eclipsing binaries are a group of detached binary systems that consists a very hot subdwarf B (sdB) type primary and a fully convective M-type secondary with periods shorter than 4 hours. Here we report the preliminary photometric study of the HW Vir-like binary NSVS14256825 based on our four years data. By analyzing the high precise BV(IR)(c) light curves of NSVS14256825 with the 2003 version of Wilson-Van Hamme code, we derived the mass ratio of this binary as q = 0.22. Assuming the mass of the primary component of NS14256825 is 0.46M(circle dot) the mass of its secondary component should be 0.1M(circle dot)(105M(Jup)) for the fully convective star. The O-C diagram of NS14256825 is shown here and the detail analysis is in progress.
收录类别CPCI
产权排序第一完成单位
会议录Astronomical Society of the Pacific (ASP) Conference Series - NINTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS
会议录出版者ASTRONOMICAL SOC PACIFIC
学科主题Astronomy & Astrophysics
会议录出版地390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
语种英语
ISBN号978-1-58381-785-8
源URL[http://ir.ynao.ac.cn/handle/114a53/5958]  
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Zhu LY(朱俐颖)
推荐引用方式
GB/T 7714
Zhu LY,Qian SB,Liu L,et al. A Preliminary Photometric Study of the HW Vir-like Binary NSVS14256825[C]. 见:9th Pacific Rim Conference on Stellar Astrophysics. Lijiang, PEOPLES R CHINA. 2011-04-14.

入库方式: OAI收割

来源:云南天文台

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