models of disk chemical evolution focusing the pure dynamical radial mixing
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2012
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Abstract
We performed N-body simulations to study the dynamical evolution of a stellar disk inside a Dark Matter (DM) halo. Our results evidence how a standard -radially decreasing- metallicity gradient produces a negative vϕ vs. [Fe/H] correlation, similar to that shown by the thin disk stars, while an inverse radial gradient generates a positive rotation-metallicity correlation, as that observed in the old thick population.
| Reference Key |
p.2012epjmodels
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|---|---|
| Authors | ;Re Fiorentin P.;Murante G.;Lattanzi M.G.;Spagna A.;Curir A. |
| Journal | utilitas mathematica |
| Year | 2012 |
| DOI |
10.1051/epjconf/20121910003
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