Fig. 1
Size-linewidth plot of M 33 clouds. Crosses indicate the velocity dispersion of the M 33 clouds as a function of the deconvolved radius Re calculated by CPROPS (cf. Sect. 3.1 Rosolowsky & Leroy 2006). Note that to obtain the full velocity width at half maximum, the dispersion needs to be multiplied by 
. The line represents the scaling law found by SRBY in the Milky Way.
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