Since Protostars and Planets VI (PPVI), our knowledge of the global properties of
protoplanetary and debris disks, as well as of young stars, has dramatically improved. At the …

Context. The evolution of protoplanetary disks is regulated by an interplay of several
processes, either internal to the system or related to the environment. As most of the stars …

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 …

As the classic viscous paradigm for protoplanetary disk accretion is challenged by the
observational evidence of low turbulence, the alternative scenario of MHD disk winds is …

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 …

How protoplanetary discs evolve remains an unanswered question. Competing theories of
viscosity and magnetohydrodynamic disc winds have been put forward as the drivers of …

Observational surveys of entire star-forming regions have provided evidence of power-law
correlations between the disc-integrated properties and the stellar mass, especially the disc …

In order to understand which mechanism is responsible for accretion in protoplanetary discs,
a robust knowledge of the observed disc radius using gas tracers such as 12CO and other …

Context. The origin of the stellar spin distribution at young ages is still unclear. Even in very
young clusters (∼ 1 Myr), a significant spread is observed in rotational periods ranging …

The time evolution of the dependence of the mass accretion rate with the stellar mass and
the disk mass represents a fundamental way to understand the evolution of protoplanetary …