Modelling the chemical evolution of the Milky Way

被引：137

作者：

Matteucci, Francesca ^{[1
]}

机构：

[1] Trieste Univ, Dept Phys, Trieste, Italy

来源：

ASTRONOMY AND ASTROPHYSICS REVIEW | 2021年 / 29卷 / 01期

关键词：

The Galaxy; Chemical evolution; Chemical abundances; NEUTRON-STAR MERGERS; METAL-POOR STARS; HIERARCHICAL GALAXY FORMATION; CHEMO-SPECTROPHOTOMETRIC EVOLUTION; GIANT BRANCH STARS; R-PROCESS; IA SUPERNOVAE; GALACTIC BULGE; ABUNDANCE GRADIENTS; SOLAR NEIGHBORHOOD;

D O I：

10.1007/s00159-021-00133-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this review, I will discuss the comparison between model results and observational data for the Milky Way, the predictive power of such models as well as their limits. Such a comparison, known as Galactic archaeology, allows us to impose constraints on stellar nucleosynthesis and timescales of formation of the various Galactic components (halo, bulge, thick disk and thin disk).

引用

页数：90

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