中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
V1224 Cas: An EL CVn-type Eclipsing Binary Consisting of a Helium White Dwarf Precursor and a Delta Scuti Pulsator

文献类型:期刊论文

作者Wang, Kun1; Luo, Changqing2; Zhang, Xiaobin2; Zhang, Bo2; Deng, Licai1,2; Luo, Zhiquan1
刊名ASTRONOMICAL JOURNAL
出版日期2018-11-01
卷号156期号:5页码:7
关键词binaries: eclipsing stars: individual (V1224 Cas) stars: variables: delta Scuti
ISSN号0004-6256
DOI10.3847/1538-3881/aade52
英文摘要We report the discovery of a new eclipsing EL CVn-type binary, consisting of a delta Sct-type pulsator and a thermally bloated low-mass pre-He white dwarf (WD). Spectroscopy and time-series BV photometry of V1224 Cas were carried out. The spectroscopy reveals a spectral type of A3 for the star. Light curve modeling indicates that V1224 Cas is a short-period detached system containing a possible low-mass WD with an effective temperature of about 9516 K. Based on the effective temperature and the surface gravity of the A-type primary star from the spectroscopic results, the absolute parameters of the components were estimated as: M-p = 2.16 +/- 0.22M(circle dot), Rp = 3.54 +/- 0.12R(circle dot), L-p = 55.9 +/- 6.9L(circle dot), M-s = 0.19 +/- 0.02M(circle dot), R-s = 0.97 +/- 0.04R(circle dot), and L-s = 6.9 +/- 0.6L(circle dot). We therefore introduce V1224 Cas as a new EL CVn-type binary candidate. The light curves in both filters all show multi-periodic pulsations, superimposed on binary effects. We performed a preliminary frequency analysis of the light residuals after removing the synthetic eclipsing curve from the original observational data. The results suggest that the rapid light variations among the light curves could be attributed to the delta Sct-type primary component. We therefore conclude that V1224 Cas is very likely a WD-delta Sct binary.
WOS关键词MULTI-PERIODIC PULSATIONS ; CLUSTER NGC 7789 ; RED-GIANT STAR ; LIGHT CURVES ; PHOTOMETRY ; SYSTEM
资助项目China Scholarship Council ; Meritocracy Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Beijing Natural Science Foundation[1184018] ; National Natural Science Foundation of China[11833002] ; National Natural Science Foundation of China[11633005] ; National Natural Science Foundation of China[11473037] ; National Natural Science Foundation of China[11373037]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000446797700004
出版者IOP PUBLISHING LTD
资助机构China Scholarship Council ; China Scholarship Council ; Meritocracy Research Funds of China West Normal University ; Meritocracy Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; Meritocracy Research Funds of China West Normal University ; Meritocracy Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; Meritocracy Research Funds of China West Normal University ; Meritocracy Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China Scholarship Council ; China Scholarship Council ; Meritocracy Research Funds of China West Normal University ; Meritocracy Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Fundamental Research Funds of China West Normal University ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Natural Science Foundation of China ; National Natural Science Foundation of China
源URL[http://ir.bao.ac.cn/handle/114a11/23034]  
专题中国科学院国家天文台
通讯作者Wang, Kun
作者单位1.China West Normal Univ, Dept Astron, Nanchong 637002, Peoples R China
2.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China
推荐引用方式
GB/T 7714
Wang, Kun,Luo, Changqing,Zhang, Xiaobin,et al. V1224 Cas: An EL CVn-type Eclipsing Binary Consisting of a Helium White Dwarf Precursor and a Delta Scuti Pulsator[J]. ASTRONOMICAL JOURNAL,2018,156(5):7.
APA Wang, Kun,Luo, Changqing,Zhang, Xiaobin,Zhang, Bo,Deng, Licai,&Luo, Zhiquan.(2018).V1224 Cas: An EL CVn-type Eclipsing Binary Consisting of a Helium White Dwarf Precursor and a Delta Scuti Pulsator.ASTRONOMICAL JOURNAL,156(5),7.
MLA Wang, Kun,et al."V1224 Cas: An EL CVn-type Eclipsing Binary Consisting of a Helium White Dwarf Precursor and a Delta Scuti Pulsator".ASTRONOMICAL JOURNAL 156.5(2018):7.

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