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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 2.

Time evolution in Model QA10x2 of (a) the mass fractions of the diffuse ( f diff, solid) and GBC ( f GBC, dotted) components, (b) the mass fractions of the cold ( f c , dashed), unstable ( f u , dotted), and warm ( f w , solid) phases within the diffuse component, (c) the density-weighted vertical scale height H, and (d) the SFR surface density Σ SFR. The initial increase of f GBC and f c stops at t = 0.1 t orb = 22 Myr when the first SN event occurs inside a massive dense cloud. The model reaches a quasi-steady state after a few tenths of an orbital time, in the sense that the physical quantities fluctuate but do not evolve secularly. Note that f diff is positively correlated with H.

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