Fig. 2.
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Upper panel: Stars-to-gas thickness ratio, hz, ⋆/hz, gas, as a function of the squared velocity-dispersion ratio, μ, for two-component isothermal slabs with different values of the midplane density ratio ξ (hz = h70%, defined by Eq. 7). Overplotted in grey is the power law, μ5/8. Lower panel: Percent residuals between the points and the power law of the upper panel.
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