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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 14.

Measured SFR surface density Σ SFR as a function of (a) Σ/ t ff, 0 and (b) Σ/ t ver for all numerical models, where t ff, 0 = (3π/(32 Gρ 0)) 1/2 and t ver = H diff/ v z, diff are computed using time-averaged values of the variables. The points and error bars give the mean and standard deviations over t/ t orb = 2–3. The dotted lines in (a) and (b) show our best fits for imposed unity slopes, Σ SFR = 0.008(Σ/ t ff, 0) and Σ SFR = 0.0025(Σ/ t ver), respectively.

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