Abstract
We performed smoothed particle hydro-dynamical simulations of isolated collapsing triaxial systems initially composed of dark matter (DM) and gas with cooling, shocks, star formation and feedback self-consistently accounted for. The initial configuration is built up as expected in the CDM scenario. We analyze the role of the initial geometry, dynamical state and mass of the DM halo on the galaxy formation and evolution. We find intriguing connections between dark and luminous matter. Multiwavelength maps shed light into different galaxy properties.
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Mazzei, P., Curir, A. Multiwavelength Maps of Simulations of Galaxy Formation. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_90
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DOI: https://doi.org/10.1007/10995020_90
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-25665-6
Online ISBN: 978-3-540-31641-1
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