Context. Previous theoretical works on planet formation around low-mass stars have often
been limited to large planets and individual systems. As current surveys routinely detect …

Aims. We investigate the evolution of protoplanetary discs (PPDs) with magnetically driven
disc winds and viscous heating. Methods. We considered an initially massive disc with~ 0.1 …

Surveys of star-forming regions reveal that the dust mass of protoplanetary discs decreases
by several orders of magnitude on timescales of a few million years. This decrease in the …

Aims. We want to find the distribution of initial conditions that best reproduces disc
observations at the population level. Methods. We first ran a parameter study using a 1D …

Context. Aims. The long-term evolution of a circumstellar disk starting from its formation and
ending in the T Tauri phase was simulated numerically with the purpose of studying the …

Context. Current research has established magnetised disc winds as a promising way of
driving accretion in protoplanetary discs. Aims. We investigate the evolution of large …

We investigate the roles of magnetically driven disc wind (MDW) and thermally driven
photoevaporative wind (PEW) in the long-time evolution of protoplanetary discs. We start …

We aim to understand the effect of stellar evolution on the evolution of protoplanetary disks.
We focus in particular on the disk evolution around intermediate-mass (IM) stars, which …

Protoplanets growing within the protoplanetary disk by pebble accretion acquire hydrostatic
gas envelopes. Due to accretion heating, the temperature in these envelopes can become …

The low water content of the terrestrial planets in the solar system suggests that the
protoplanets formed within the water snow line. Accurate prediction of the snow line location …