Fig. 4

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Model evolution for a case with log[Mgas,0(M⊙)] = 6.3, Rcl = 25.7 pc, ϵff = 0.3, and for the IZw 18 metallicity. First plot from top to bottom: shell radius (left y-axis), shell velocity (right y-axis). Second: shell mass (Msh), stellar mass formed from core star formation (Msc,c), and total stellar mass (Msc). Third: the outward force produced by the thermal energy (
, dashed) and the total inward forces (
, solid). Fourth, bottom right panel: mechanical power (solid) produced by the stellar feedback and the cooling rate (dashed).
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