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Fig. 6


Fiducial model and variations of the most important parameters: fragmentation power-law index ξ, threshold fragmentation velocity uf, turbulence parameters αt, surface density Σg, particle internal density ρs, and mid-plane temperature T. The shape of the vertically integrated size distributions does not depend on the stellar mass or the distance to the star (only via the radial dependence of the parameters above).

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