Star formation in a multi-phase interstellar medium

Details Star formation in a multi-phase interstellar medium Star formation in a multi-phase interstellar medium

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.284..833s&link_type=abstract

Astrophysics and Space Science, v. 284, Issue 2, p. 833-836 (2003).

Astronomy and Astrophysics

Astrophysics

Hydrodynamics, Interstellar Medium, Star Formation, Feedback

Scientific paper

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.

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