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Asteroseismology of DAV star EC14012-1446, mode identification and model fittings
Chen YH(陈彦辉)1,2,3; Li Y(李焱)1,2
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2014-10-01
卷号443期号:4页码:3477-3485
DOI10.1093/mnras/stu1409
产权排序第1完成单位
收录类别SCI
关键词Asteroseismology Stars: Individual: Ec14012-1446 White Dwarfs
摘要

EC14012-1446 was observed by Handler et al. in 2004 April, June, 2005 May, and 2007 April, and by Provencal et al. in 2008. We review the observations together and obtain 34 independent frequencies. According to the frequency splitting and the asymptotic period spacing law, we identify 6 l = 1 modes, 4 l = 2 modes, 5 l = 3 modes, 10 l = 1 or 2 modes. Grids of white dwarf models are generated by WDEC with H, He, C, O diffusion in a four-parameter space. The core compositions are directly from white dwarf models generated by MESA. The best-fitting model has M-* = 0.710 M-circle dot, T-eff = 12 200 K, log(M-He/M-*) = -2.5, log(M-H/M-*) = -7.0, log g = 8.261, and phi = 3.185 s. There are four, two, and one modes identified as trapped in H envelope for observed l = 1, 2, and 3 modes, respectively. Trapped modes jump the queue of uniform period spacing.

资助项目Knowledge Innovation Key Programme of the University of Chinese Academy of Sciences[KJCX2-YW-T24] ; [XDB09010202]
项目资助者Knowledge Innovation Key Programme of the University of Chinese Academy of Sciences[KJCX2-YW-T24] ; [XDB09010202]
语种英语
学科领域天文学 ; 恒星与银河系 ; 恒星物理学
文章类型Article
出版者OXFORD UNIV PRESS
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
ISSN0035-8711
URL查看原文
归档日期2014-10-13
WOS记录号WOS:000342922100048
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]ZZ CETI STARS ; THERMONUCLEAR REACTION-RATES ; WHOLE EARTH TELESCOPE ; WHITE-DWARFS ; EVOLUTIONARY MODELS ; INSTABILITY STRIP ; SPECTROSCOPY ; OSCILLATIONS
引用统计
被引频次:7[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/114a53/5236
专题恒星物理研究组
中国科学院天体结构与演化重点实验室
通讯作者Chen YH(陈彦辉)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
3.University of Chinese Academy of Sciences, Beijing 100049, 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
Chen YH,Li Y. Asteroseismology of DAV star EC14012-1446, mode identification and model fittings[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,443(4):3477-3485.
APA Chen YH,&Li Y.(2014).Asteroseismology of DAV star EC14012-1446, mode identification and model fittings.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,443(4),3477-3485.
MLA Chen YH,et al."Asteroseismology of DAV star EC14012-1446, mode identification and model fittings".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 443.4(2014):3477-3485.
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