Preliminary identification of the observed pulsation modes of ZZ Ceti star KUV 03442+0719

doi:10.1016/j.newast.2014.04.006

YNAO OpenIR > 大样本恒星演化研究组

	Preliminary identification of the observed pulsation modes of ZZ Ceti star KUV 03442+0719
	Su J(苏杰)1,2,3 ; Li Y(李焱)1,2 ; Fu, JN 4
发表期刊	NEW ASTRONOMY
	2014-11
卷号	33 页码:52-56
DOI	10.1016/j.newast.2014.04.006
产权排序	第1完成单位
收录类别	SCI
关键词	Oscillations White Dwarfs
摘要	KUV 03442+0719 is a ZZ Ceti star originally discovered in 2005. We performed observations for it in 2010, 2011 and 2012. From the three years' Fourier transform spectra, a total number of 43 pulsation periods are detected. We found out a set of complete quintuplets, five sets of incomplete quintuplets and two sets of incomplete triplets among these periods. They are interpreted as rotational splits of l = 2 and l = 1 modes. We thus derive a mean rotation period of 6.71 +/- 0.11 h from the values of splitting spacing. We perform asymptotic analysis to get preliminary identification of the observed pulsation modes.
资助项目	Knowledge Innovation Program of the Chinese Academy of Sciences[KJCX2-YW-T24] ; National Natural Science Foundation of China[11273054] ; Astronomy of National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences[U1231202] ; National Basic Research Program of China(973 Program)[2014CB845700] ; National Basic Research Program of China(973 Program)[2013CB834900]
项目资助者	Knowledge Innovation Program of the Chinese Academy of Sciences[KJCX2-YW-T24] ; National Natural Science Foundation of China[11273054] ; Astronomy of National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences[U1231202] ; National Basic Research Program of China(973 Program)[2014CB845700, 2013CB834900]
语种	英语
学科领域	天文学 ; 恒星与银河系 ; 恒星物理学 ; 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	2014-06-12
WOS记录号	WOS:000337879500007
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	INSTABILITY STRIP ; WHITE-DWARFS ; ASTEROSEISMOLOGY ; DISCOVERY
引用统计	被引频次：6[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/114a53/4571
专题	大样本恒星演化研究组中国科学院天体结构与演化重点实验室
通讯作者	Su J(苏杰)
作者单位	1.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, China 3.University of Chinese Academy of Sciences, Beijing 100049, China 4.Department of Astronomy, Beijing Normal University, Beijing 100875, 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	Su J,Li Y,Fu, JN. Preliminary identification of the observed pulsation modes of ZZ Ceti star KUV 03442+0719[J]. NEW ASTRONOMY,2014,33:52-56.
APA	Su J,Li Y,&Fu, JN.(2014).Preliminary identification of the observed pulsation modes of ZZ Ceti star KUV 03442+0719.NEW ASTRONOMY,33,52-56.
MLA	Su J,et al."Preliminary identification of the observed pulsation modes of ZZ Ceti star KUV 03442+0719".NEW ASTRONOMY 33(2014):52-56.

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