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- W223574423 abstract "We performed smooth particle hydrodynamic (SPH) simulations including star formation and self-consistent chemo-photometric evolutionary population synthesis (EPS) predictions from far-UV to 1 mm, of isolated collapsing triaxial systems initially composed of dark matter (DM) and gas. The dependence of the system evolution on some parameters so far unexplored, such as its total mass, initial geometry, dynamical state and the effects of different baryonic to DM mass ratios have been investigated. We find important connections between dark and luminous matter." @default.
- W223574423 created "2016-06-24" @default.
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- W223574423 date "2003-01-01" @default.
- W223574423 modified "2023-09-26" @default.
- W223574423 title "The history of star formation in galaxies. Insights from SPH simulations of triaxial collapsing systems" @default.
- W223574423 hasPublicationYear "2003" @default.
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