中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Low-mass Pre-He White Dwarf Stars in Kepler Eclipsing Binaries with Multi-periodic Pulsations

文献类型:期刊论文

作者Zhang, X. B.1; Fu, J. N.2; Liu, N.2; Luo, C. Q.1; Ren, A. B.2
刊名ASTROPHYSICAL JOURNAL
出版日期2017-12-01
卷号850期号:2页码:8
ISSN号0004-637X
关键词binaries: eclipsing stars: individual (KIC 10989032, KIC 8087799) stars: oscillations white dwarfs
DOI10.3847/1538-4357/aa9577
英文摘要We report the discovery of two thermally bloated low-mass pre-He white dwarfs (WDs) in two eclipsing binaries, KIC 10989032 and KIC 8087799. Based on the Kepler long-cadence photometry, we determined comprehensive photometric solutions of the two binary systems. The light curve analysis reveals that KIC 10989032 is a partially eclipsed detached binary system containing a probable low-mass WD with the temperature of about 10,300 K. Having a WD with the temperature of about 13,300, KKIC 8087799 is typical of an EL CVn system. By utilizing radial velocity measurements available for the A-type primary star of KIC 10989032, the mass and radius of the WD component are determined to be 0.24 +/- 0.02 M-circle dot and 0.50 +/- 0.01 R-circle dot, respectively. The values of mass and radius of the WD in KIC 8087799 are estimated as 0.16 +/- 0.02M(circle dot) and 0.21 +/- 0.01 R-circle dot, respectively, according to the effective temperature and mean density of the A-type star derived from the photometric solution. We therefore introduce KIC 10989032 and KIC 8087799 as the eleventh and twelfth dA+ WD eclipsing binaries in the Kepler field. Moreover, both binaries display marked multi-periodic pulsations superimposed on binary effects. A preliminary frequency analysis is applied to the light residuals when subtracting the synthetic eclipsing light curves from the observations, revealing that the light pulsations of the two systems are both due to the delta Sct-type primaries. We hence classify KIC 10989032 and KIC 8087799 as two WD+delta Sct binaries.
WOS关键词DELTA-SCUTI STARS ; RED-GIANT STAR ; SX PHE STARS ; LIGHT CURVES ; SYSTEM
资助项目National Natural Science Foundation of China (NSFC) ; NSFC/CAS Joint Fund of Astronomy[11373037] ; NSFC/CAS Joint Fund of Astronomy[U1331121] ; National Natural Science Foundation of China (NSFC)[11673003] ; National Basic Research Program of China (973 Program)[2014CB845700] ; National Basic Research Program of China (973 Program)[2013CB834900]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000425473800001
资助机构National Natural Science Foundation of China (NSFC) ; NSFC/CAS Joint Fund of Astronomy ; National Natural Science Foundation of China (NSFC) ; National Basic Research Program of China (973 Program) ; National Natural Science Foundation of China (NSFC) ; NSFC/CAS Joint Fund of Astronomy ; National Natural Science Foundation of China (NSFC) ; National Basic Research Program of China (973 Program) ; National Natural Science Foundation of China (NSFC) ; NSFC/CAS Joint Fund of Astronomy ; National Natural Science Foundation of China (NSFC) ; National Basic Research Program of China (973 Program) ; National Natural Science Foundation of China (NSFC) ; NSFC/CAS Joint Fund of Astronomy ; National Natural Science Foundation of China (NSFC) ; National Basic Research Program of China (973 Program)
源URL[http://ir.bao.ac.cn/handle/114a11/35813]  
专题中国科学院国家天文台
通讯作者Zhang, X. B.
作者单位1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
2.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
推荐引用方式
GB/T 7714
Zhang, X. B.,Fu, J. N.,Liu, N.,et al. Low-mass Pre-He White Dwarf Stars in Kepler Eclipsing Binaries with Multi-periodic Pulsations[J]. ASTROPHYSICAL JOURNAL,2017,850(2):8.
APA Zhang, X. B.,Fu, J. N.,Liu, N.,Luo, C. Q.,&Ren, A. B..(2017).Low-mass Pre-He White Dwarf Stars in Kepler Eclipsing Binaries with Multi-periodic Pulsations.ASTROPHYSICAL JOURNAL,850(2),8.
MLA Zhang, X. B.,et al."Low-mass Pre-He White Dwarf Stars in Kepler Eclipsing Binaries with Multi-periodic Pulsations".ASTROPHYSICAL JOURNAL 850.2(2017):8.

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来源:国家天文台

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