Toward a population synthesis of disks and planets - I. Evolution of dust with entrainment in winds and radiation pressure

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Fig. 6

Dust and pebble mass (top) and cumulative entrained mass (bottom) evolution for different X-ray luminosities. L_X controls the strength of internally driven photoevaporation in our prescription from Picogna et al. (2021). Except for the nominal case, we use reduced F_FUV.

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