当前位置:
X-MOL 学术
›
Astron. Astrophys. Rev.
›
论文详情
Our official English website, www.x-mol.net, welcomes your
feedback! (Note: you will need to create a separate account there.)
Modelling the chemical evolution of the Milky Way
The Astronomy and Astrophysics Review ( IF 27.8 ) Pub Date : 2021-08-27 , DOI: 10.1007/s00159-021-00133-8 Francesca Matteucci 1
中文翻译:
模拟银河系的化学演化
更新日期:2021-08-27
The Astronomy and Astrophysics Review ( IF 27.8 ) Pub Date : 2021-08-27 , DOI: 10.1007/s00159-021-00133-8 Francesca Matteucci 1
Affiliation
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).
中文翻译:
模拟银河系的化学演化
在这篇评论中,我将讨论银河系模型结果与观测数据之间的比较、此类模型的预测能力及其局限性。这种被称为银河考古学的比较使我们能够对恒星核合成和各种银河组成部分(晕、核球、厚盘和薄盘)形成的时间尺度施加限制。