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Regulation of Star Formation Rates in Multiphase Galactic Disks: Numerical Tests of the Thermal/Dynamical Equilibrium Model

ASTROPHYSICAL JOURNAL, no. 1 (2011)

Cited by: 101|Views3

Abstract

We use vertically resolved numerical hydrodynamic simulations to study star formation and the interstellar medium (ISM) in galactic disks. We focus on outer-disk regions where diffuse HI dominates, with gas surface densities Sigma = 3-20 M-circle dot pc(-2) and star-plus-dark matter volume densities rho(sd) = 0.003-0.5 M-circle dot pc(-3)...More

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