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...

書誌詳細
主要な著者:	Powell, L, Bournaud, F, Chapon, D, Devriendt, J, Slyz, A, Teyssier, R
フォーマット:	Journal article
出版事項:	Cambridge University Press 2011

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