Fig. A.1

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Time evolution of a disc around a 3M⊙ star computed with this paper version of PLANETALP. As in fig. 8 of Kunitomo et al. (2021), the panels on the left show the time evolution of the gas surface density (top) and the midplane temperature (bottom) profiles. The panels on the right show the time evolution of the mass accretion rate, Ṁacc, and the mass-loss rates by X-ray and FUV photoevaporation (top), and the evolution of the disc mass and the time-integrated masses of accretion and photoevaporation (FUV and X-ray). The thick grey curves in each panel show the results from K21
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