New photometric investigation of eclipsing binary NSVS 10653195

doi:10.1016/j.newast.2015.04.009

YNAO OpenIR > 双星与变星研究组

	New photometric investigation of eclipsing binary NSVS 10653195
	Zhang B(张斌)1,2,3 ; Qian SB(钱声帮)1,2,3 ; Liao WP(廖文萍)1,2 ; Zhang J(张嘉)1,2 ; Liu NP(刘念平)1,2 ; Wang JJ(王晶晶)1,2
发表期刊	NEW ASTRONOMY
	2015-11
卷号	41 页码:37-41
DOI	10.1016/j.newast.2015.04.009
产权排序	第1完成单位
收录类别	SCI
关键词	Binary Eclipsing Binary Orbital Period Light Curve
摘要	New CCD photometric light curves of the low-mass binary system NSVS 10653195 are presented. Our complete B, V, R-c and I-c-band light curves show a remarkable out-eclipsing distortion. This phenomenon suggests that the components of the system may be active. The photometric solutions with star-spot were derived by using the 2013 version of the Wilson-Devinney (WD) code. Based on all available times of light minimum, we analyzed the orbital period changes. The O-C diagram reveals that the period of NSVS 10653195 is decreasing at a rate of dP/dt = -2.79 x 10(-7) days yr(-1), which is probably caused by angular momentum loss. (C) 2015 Elsevier B.V. All rights reserved,
资助项目	Yunnan Province[2012HC011] ; Chinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[11325315] ; Chinese Natural Science Foundation[11103074] ; Strategic Priority Research Program The Emergence of Cosmological Structures of the Chinese Academy of Sciences[XDB09010202]
项目资助者	Yunnan Province[2012HC011] ; Chinese Natural Science Foundation[11133007, 11325315, 11103074] ; Strategic Priority Research Program The Emergence of Cosmological Structures of the Chinese Academy of Sciences[XDB09010202]
语种	英语
学科领域	天文学 ; 恒星与银河系 ; 恒星天文学 ; 恒星形成与演化
文章类型	Article
出版者	ELSEVIER SCIENCE BV
出版地	PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
ISSN	1384-1076
URL	查看原文
归档日期	2015-10-23
WOS记录号	WOS:000368045200007
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	LOW-MASS STARS ; MAGNETIC ACTIVITY ; VELOCITY CURVES ; CLOSE-BINARY ; LIGHT CURVES ; MODELS ; EVOLUTION ; CYGNI
引用统计	被引频次：8[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/9400
专题	双星与变星研究组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, P.O. Box 110, Kunming 650216, PR China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, PR China 3.Graduate University of Chinese Academy of sciences, Beijing, PR China
第一作者单位	中国科学院云南天文台
通讯作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Zhang B,Qian SB,Liao WP,et al. New photometric investigation of eclipsing binary NSVS 10653195[J]. NEW ASTRONOMY,2015,41:37-41.
APA	Zhang B,Qian SB,Liao WP,Zhang J,Liu NP,&Wang JJ.(2015).New photometric investigation of eclipsing binary NSVS 10653195.NEW ASTRONOMY,41,37-41.
MLA	Zhang B,et al."New photometric investigation of eclipsing binary NSVS 10653195".NEW ASTRONOMY 41(2015):37-41.

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