Fig. C.1.
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Radial averages in M33 as a function of galactocentric distance R. From top to bottom: Star formation rate surface density, ΣSFR, using various indicators (see Appendix D for details), the effective SFE, ΣSFR/ΣH2, the midplane pressures Phy, PBR0≡ PDE*, and P
, the ratio between the stellar and gaseous pressure terms, P2/P1, in PDE* and Phy, the stellar to gas volume density ratio ρs/ρg, the dust to total gas mass surface density ratio Σdust/Σg, the orbital, and epicyclic times to, te, and the Toomre parameter Q for a thin disk with or without considering the dark matter gravity. The gray dashed lines indicate unity ratios.
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