中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The barium-to-iron enrichment versus age relation of ancient disc stars

文献类型:期刊论文

作者Fuhrmann, K.; Chini, R.; Kaderhandt, L.; Chen, Z.; Lachaume, R.
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2017
卷号471期号:3页码:3768-3774
英文摘要We report an intrinsically precise relation of the barium-to-iron enrichment as a function of age for a local, volume-complete (N = 30) sample of ancient Population II (tau >= 12 Gyr) and intermediate-disc stars (tau similar or equal to 10 Gyr), which suggests a common, r-process-dominated nucleosynthesis site for both elements in the early stages of the Milky Way. Deviants from this empirical relation are to a large extent identified as formerly known or new blue straggler stars. We report in particular the striking case of the Population II star HD159062, whose barium overabundance is difficult to explain without wind accretion of s-process material from a former asymptotic giant branch (AGB) primary that very likely survived as a white dwarf companion. The weak but significant barium enhancement that we measure for HR3578 and 104 Tau also suggests that both may be accompanied by faint degenerate companions. If confirmed through precision astrometry or direct imaging observations, this would mean a very efficient method to uncover ancient stellar remnant companions around solar-type stars.
语种英语
源URL[http://libir.pmo.ac.cn/handle/332002/17334]  
专题中国科学院紫金山天文台
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Fuhrmann, K.,Chini, R.,Kaderhandt, L.,et al. The barium-to-iron enrichment versus age relation of ancient disc stars[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,471(3):3768-3774.
APA Fuhrmann, K.,Chini, R.,Kaderhandt, L.,Chen, Z.,&Lachaume, R..(2017).The barium-to-iron enrichment versus age relation of ancient disc stars.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,471(3),3768-3774.
MLA Fuhrmann, K.,et al."The barium-to-iron enrichment versus age relation of ancient disc stars".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 471.3(2017):3768-3774.

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来源:紫金山天文台

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