Chemo-dynamical simulations of galaxies
We predict the frequency distribution of elemental abundance ratios from Carbon to Zinc as a functions of time and location, which can be directly compared with the next generation of the galactic archeology project such as the HERMES. We perform the chemodynamical simulations of a Milky Way-type galaxy from a CDM initial condition, using a self-consistent hydrodynamical code with supernova feedback and chemical enrichment. In the simulated galaxy, the kinematical and chemical properties of the...[Show more]
|Collections||ANU Research Publications|
|Source:||AIP Conference Proceedings Volume 1269: THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG 2010|
|01_Kobayashi_Chemo-dynamical_simulations_of_2010.pdf||1.63 MB||Adobe PDF||Request a copy|
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