中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Abundances of 23 field RR Lyrae stars

文献类型:期刊论文

作者Liu, Shu1,2; Zhao, Gang1; Chen, Yu-Qin1; Takeda, Yoichi3; Honda, Satoshi4; Chen Yuqin; Gang Zhao; Shu Liu
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2013-11-01
卷号13期号:11页码:1307-1329
关键词techniques: spectroscopic stars: abundances stars: variables: RR Lyrae
英文摘要We present stellar parameters and abundances of 15 elements (Na, Mg, Al, Si, Ca, Sc, Ti, V, Cr, Mn, Fe, Ni, Cu, Y and Ba) for 23 field RR Lyrae variables based on high-resolution (R similar to 60 000) and high signal-to-noise (S/N similar to 2 0 0) spectra obtained using the High Dispersion Spectrograph on the Subaru Telescope. Six stars in the sample have more than one spectrum observed at different pulsation phases. The derived abundance ratios of [X/Fe] for 14 elements (except for Ba) do not vary during the pulsation cycle. An interesting curve of [Ba/Fe] versus phase is detected for the first time and it shows decreasing [Ba/Fe] with increasing temperature at a given metallicity. Combining with data in the literature, abundances of most RR Lyrae stars as a function of [Fe/H] follow the same trends as those of dwarf stars, but [Sc/Fe] and [Y/Fe] ratios of RR Lyrae stars at solar metallicity are lower than those of dwarf stars. The kinematics of RR Lyrae stars indicate that three comparatively metal-rich RR Lyrae stars might originate from the thick disk and they show higher [alpha/Fe] ratios than RR Lyrae stars with thin disk kinematics. Among 23 RR Lyrae stars, two special objects are found with abnormal abundances; TV Lib has high [alpha/Fe], [Sc/Fe], [Y/Fe] and [Ba/Fe] ratios while TW Her has solar [alpha/Fe] but significantly lower [Sc/Fe], [Y/Fe] and [Ba/Fe] ratios as compared with other RR Lyrae stars.
收录类别SCI
语种英语
WOS记录号WOS:000326281500003
源URL[http://ir.bao.ac.cn/handle/114a11/5831]  
专题国家天文台_光学天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
2.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
3.Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
4.Univ Hyogo, Ctr Astron, Nishi Harima Astron Observ, Sayo, Hyogo 6795313, Japan
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GB/T 7714
Liu, Shu,Zhao, Gang,Chen, Yu-Qin,et al. Abundances of 23 field RR Lyrae stars[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2013,13(11):1307-1329.
APA Liu, Shu.,Zhao, Gang.,Chen, Yu-Qin.,Takeda, Yoichi.,Honda, Satoshi.,...&Shu Liu.(2013).Abundances of 23 field RR Lyrae stars.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,13(11),1307-1329.
MLA Liu, Shu,et al."Abundances of 23 field RR Lyrae stars".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 13.11(2013):1307-1329.

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来源:国家天文台

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