Galactic chemical evolution

被引：44

作者：

Gibson, BK ^{[1
]}

Fenner, Y ^{[1
]}

Renda, A ^{[1
]}

Kawata, D ^{[1
]}

Lee, HC ^{[1
]}

机构：

[1] Swineburne Univ, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2003年 / 20卷 / 04期

关键词：

Galaxy : abundances; Galaxy : evolution; Galaxy : formation; Galaxy : kinematics and dynamics; methods : N-body simulations;

D O I：

10.1071/AS03052

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The primary present-day observables upon which theories of galaxy evolution are based are a system's morphology, dynamics, colour, and chemistry. Individually, each provides an important constraint to any given model; in concert, the four represent a fundamental ( intractable) boundary condition for chemodynamical simulations. We review the current state-of-the-art semi-analytical and chemodynamical models for the MilkyWay, emphasising the strengths and weaknesses of both approaches.

引用

页码：401 / 415

页数：15

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