Star formation in a multi-phase interstellar medium
This contribution reports on our first efforts to simulate a multiphase interstellar medium on a kiloparsec scale in three dimensions with the stars and gas modeled self-consistently. Starting from inhomogenous initial conditions, our closed box simulations follow the gas as it cools and collapses u...
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| Aineistotyyppi: | Conference item |
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2003
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