Galactic star formation in parsec-scale resolution simulations
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...
| Главные авторы: | , , , , , |
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| Формат: | Journal article |
| Опубликовано: |
Cambridge University Press
2011
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