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Fig. 15
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Disc gas mass (left) and accretion rate (right) over the course of 10 Myr for an example 100 MJ, 100 au disc around a solar-mass star undergoing viscous evolution (α = 10−3) and photoevaporation using the mass-loss prescription of Picogna et al. (2021) (black) or from this work (blue).
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