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University of Birmingham > Talks@bham > Astrophysics Talks Series > Chemodynamical simulations of galaxies
Chemodynamical simulations of galaxiesAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Alastair Sanderson. The formation and evolutionary history of galaxies are imprinted in the elemental abundance ratios of stars. I am simulating the chemodynamical evolution of galaxies using my hydrodynamical code that includes star formation and chemical enrichment from core-collapse and Type Ia supernovae, and AGB stars. It is possible to predict the time/redshift evolution of the spatial distribution of elements in the Universe and to compare with observations of nearby and distant galaxies. In this talk, I will discuss the mass-metallicity relation of galaxies, the stellar populations of the Galactic bulge and disk, and the elemental abundances of metal-poor Damped Lyman alpha systems. This talk is part of the Astrophysics Talks Series series. This talk is included in these lists:Note that ex-directory lists are not shown. |
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