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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 9.

Measured vs. estimated values of (a) midplane number densities and (b) disk scale heights of the diffuse gas. The points and error bars give the mean and standard deviations over t/ t orb = 2–3. The estimated midplane number density n 0, DE ≡ ρ 0, DE/(1.4 m p ) and scale height H diff, DE are obtained from dynamical equilibrium as Equations (39) and (40), respectively. The dashed lines show our best fits n 0 = 1.4 n 0, DE and H diff = 0.87 H diff, DE for imposed unity slopes, while the dotted lines indicate one-to-one correspondence.

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