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- W1944492780 abstract "We highlight two research strands related to our ongoing chemodynamical Galactic Archaeology efforts: (i) the spatio-temporal infall rate of gas onto the disk, drawing analogies with the infall behaviour imposed by classical galactic chemical evolution models of inside-out disk growth; (ii) the radial age gradient predicted by spectrophometric models of disk galaxies. In relation to (i), at low-redshift, we find that half of the infall onto the disk is gas associated with the corona, while half can be associated with cooler gas streams; we also find that gas enters the disk preferentially orthogonal to the system, rather than in-plane. In relation to (ii), we recover age gradient troughs/inflections consistent with those observed in nature, without recourse to radial migrations." @default.
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- W1944492780 date "2012-04-06" @default.
- W1944492780 modified "2023-10-16" @default.
- W1944492780 title "Gas and Metal Distributions within Simulated Disk Galaxies" @default.
- W1944492780 hasPublicationYear "2012" @default.
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