Galactic winds - How to launch galactic outflows in typical Lyman-break galaxies

Monthly Notices of the Royal Astronomical Society(2013)

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Abstract
We perform hydrodynamical simulations of a young galactic disc embedded in a hot gaseous halo using parameters typical for Lyman-break galaxies (LBGs). We take into account the (static) gravitational potentials due to a dark matter halo, a stellar bulge and a disc of stars and gas. Star formation is treated by a local Kennicutt–Schmidt law. We simplify the structure of the interstellar medium (ISM...
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Key words
methods: numerical,ISM: bubbles,galaxies: evolution,galaxies: haloes,galaxies: high-redshift,galaxies: ISM
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