中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
numericalsimulationofapossibleoriginofthepositiveradialmetallicitygradientofthethickdisk

文献类型:期刊论文

作者Rahimi Awat1; Carrell Kenneth1; Kawata Daisuke2
刊名researchinastronomyandastrophysics
出版日期2014
卷号14期号:11页码:1406
ISSN号1674-4527
英文摘要We analyze the radial and vertical metallicity and alpha/Fe gradients of the disk stars of a disk galaxy simulated in a fully cosmological setting with the chemo-dynamical galaxy evolution code GCD+. We study how the radial abundance gradients vary as a function of height above the plane and find that the metallicity (alpha/Fe) gradient becomes more positive (negative) with increasing height, changing sign around 1.5 kpc above the plane. At the largest vertical height (2 2 kpc at the outer region, because of the lower gravitational restoring force of the disk, i.e. flaring. As a result, the fraction of younger stars with higher metallicity due to the age-metallicity relation becomes higher at the outer radii, which makes the median metallicity higher at the outer radii. Combining this result with the recently observed age-metallicity and age-velocity dispersion relation for the Milky Way thick disk stars suggested by Haywood et al., we argue that the observed (small) positive radial metallicity gradient at large heights of the Milky Way disk stars can be explained by flaring of the younger thick and/or thin disk stars.
资助项目[National Astronomical Observatories, Chinese Academy of Sciences] ; [Chinese Academy of Sciences Fellowships for Young International Scientists] ; [National Natural Science Foundation of China (NSFC)]
语种英语
源URL[http://ir.bao.ac.cn/handle/114a11/51595]  
专题中国科学院国家天文台
作者单位1.中国科学院国家天文台
2.伦敦大学学院
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Rahimi Awat,Carrell Kenneth,Kawata Daisuke. numericalsimulationofapossibleoriginofthepositiveradialmetallicitygradientofthethickdisk[J]. researchinastronomyandastrophysics,2014,14(11):1406.
APA Rahimi Awat,Carrell Kenneth,&Kawata Daisuke.(2014).numericalsimulationofapossibleoriginofthepositiveradialmetallicitygradientofthethickdisk.researchinastronomyandastrophysics,14(11),1406.
MLA Rahimi Awat,et al."numericalsimulationofapossibleoriginofthepositiveradialmetallicitygradientofthethickdisk".researchinastronomyandastrophysics 14.11(2014):1406.

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来源:国家天文台

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