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

  • Authors: Chang-Goo Kim, Woong-Tae Kim, and Eve C. Ostriker

Kim, Kim, & Ostriker 2011 The Astrophysical Journal 743 25.

  • Provider: AAS Journals

Caption: Figure 4.

(a) Distribution of gas in the nP/ k B plane for Model QA10x2, averaged over t/ t orb = 2–3. The color bar gives the mass fraction in logarithmic scale. The solid curve marks the locus of thermal equilibrium at the mean heating rate of langΓ rang = 0.76Γ 0. Mass-weighted (thick) and volume-weighted (thin) probability distribution functions are shown for (b) thermal pressure and (c) number density. The vertical dotted lines in (b) and (c) mark the mean midplane thermal pressure and number density, respectively, of the diffuse gas. These results show that the system evolves to a state in which approximate two-phase thermal equilibrium at a common pressure holds for the atomic gas.

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