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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 8.

Top: midplane (a) total and (b) thermal pressures of the diffuse gas as functions of . The points and error bars give the mean and standard deviations over t/ t orb = 2–3. The dotted lines in upper panels show fits P tot/ k B = 9.9 × 10 3 cm −3 K(Σ/10  M  pc −2)(ρ sd/0.1  M  pc −3) 1/2 and P th/ k B = 2.2 × 10 3 cm −3 K(Σ/10  M  pc −2)(ρ sd/0.1  M  pc −3) 1/2, respectively. Bottom: relative differences between measured midplane pressures and the dynamical equilibrium estimates using Equation (35). The mean midplane pressure P tot varies only 13% relative to P tot, DE, showing that vertical dynamical equilibrium is an excellent approximation.

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