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Star formation in a multi-phase interstellar medium

Abstract:
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 under its own self-gravity to form stars which eventually return material and energy back through supernovae explosions and winds.
Publication status:
Published

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Publisher copy:
10.1023/A:1024006213407
Host title:
ASTROPHYSICS AND SPACE SCIENCE
Volume:
284
Issue:
2
Pages:
833-836
Publication date:
2003-01-01
DOI:
ISSN:
0004-640X
Keywords:
Pubs id:
pubs:15112
UUID:
uuid:3d8cf65f-1736-4165-875f-4296ca14fe2c
Local pid:
pubs:15112
Source identifiers:
15112
Deposit date:
2012-12-19

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