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Galactic Chemical Evolution
Published online by Cambridge University Press: 05 March 2013
Abstract
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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 Milky Way, emphasising the strengths and weaknesses of both approaches.
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- Sixth Torino Workshop
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- Copyright © Astronomical Society of Australia 2003
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