Galactic star formation in parsec-scale resolution simulations

Galactic star formation in parsec-scale resolution simulations

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The interstellar medium (ISM) in galaxies is multiphase and cloudy, with stars forming in the very dense, cold gas found in Giant Molecular Clouds (GMCs). Simulating the evolution of an entire galaxy, however, is a computational problem which covers many orders of magnitude, so many simulations can...

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Detalles Bibliográficos
Main Authors:	Powell, L, Bournaud, F, Chapon, D, Devriendt, J, Slyz, A, Teyssier, R
Formato:	Journal article
Publicado:	Cambridge University Press 2011

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