Radial migration and chemical evolution in the Milky Way

被引：1
作者：
Prantzos, N. [1 ,2 ]
机构：
[1] CNRAS UMP 7095, Inst Astrophys Paris, Paris, France
[2] Univ Paris 06, F-75252 Paris 05, France
来源：
ASTRONOMISCHE NACHRICHTEN | 2016年 / 337卷 / 8-9期
关键词：
Galaxy: abundances; Galaxy: evolution; Galaxy: kinematics and dynamics; N-body simulations; STELLAR DISK; STARS; ABUNDANCE;
D O I：
10.1002/asna.201612406
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The role of radial migration on the chemical evolution of the Milky Way is studied with semi-analytical models of disk evolution, using several new/updated ingredients and parametrized prescriptions for blurring and churning. It is found that radial migration impacts on several properties of the local disk (shape and dispersion of the age-metallicity relation, metallicity distribution), it may explain some chemical properties of the local thin and thick disks (i.e. the two-branch shape of the O/Fe vs. Fe/H relation) and it affects the past abundance profiles of the stellar population. (C) 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
引用
收藏
页码：953 / 956
页数：4
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