Comparing Cosmological Hydrodynamic Simulations with Observations of High-Redshift Galaxy Formation

Comparing Cosmological Hydrodynamic Simulations with Observations of High-Redshift Galaxy Formation

We use cosmological hydrodynamic simulations to study the impact of out-flows and radiative feedback on high-redshift galaxies. For outflows, we consider simulations that assume (i) no winds, (ii) a .constant-wind. model in which the mass-loading factor and outflow speed are constant, and (iii) &quo...

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Bibliographic Details
Main Author: Finlator, Kristian Markwart
Other Authors: Dave, Romeel
Language:EN
Published: The University of Arizona. 2009
Subjects:
cosmology: theory
galaxies: evolution
galaxies: formation
galaxies: high-redshift
methods: numerical
radiation transport
Online Access:http://hdl.handle.net/10150/195788

Internet

http://hdl.handle.net/10150/195788

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