
%0 Journal Article
%A Gibson, Brad K. 
%A Fenner, Yeshe 
%A Renda, Agostino 
%A Kawata, Daisuke 
%A Lee, Hyun-chul 
%T Galactic Chemical Evolution
%J Publications of the Astronomical Society of Australia
%D 2003/12/24
%V 20
%N 4
%P 401-415
%K Galaxy: abundances &#8212; Galaxy: evolution &#8212; Galaxy: formation &#8212; Galaxy: kinematics and dynamics &#8212; methods: N-body simulations
%R https://doi.org/10.1071/AS03052
%U https://www.publish.csiro.au/paper/AS03052 
%X The primary present-day observables upon which theories of galaxy evolution are based are a system&#8217;s morphology, dynamics, colour, and chemistry. Individually, each provides an important constraint to any given model&#x003B; 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 Milky Way, emphasising the strengths and weaknesses of both approaches. 
