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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 6.

(a) The vertical turbulent velocity dispersion of the diffuse gas v z, diff, (b) the total (turbulent+thermal) velocity dispersion of the diffuse gas σ z, diff, and (c) the total velocity dispersion of all gas σ z, as functions of the SFR surface density Σ SFR for all models except Series R. The points and error bars give the mean and standard deviations over t/ t orb = 2–3. For the whole set of models shown in this figure, v z, diff = 6.8 ± 0.6 km s −1, σ z, diff = 7.7 ± 0.6 km s −1, and σ z = 7.0 ± 0.4 km s −1. The dotted lines in all panels show 7 km s −1 for reference.

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