… and planetesimal formation at early evolutionary stages when the influence of the disc's
self-… behaviour of particles embedded in a self-gravitating disc using a local shearing sheet …

… In this Letter, we show that if planetesimals form in spiral features in self-gravitating discs, as
… in realistic protostellar discs, this process will be restricted to the outer regions of the disc (ie …

… We study particle dynamics in self-gravitating gaseous discs … in the gaseous component of
the disc due to a gravitational … allow the solid component of the disc to collapse under its own …

… The other perturbation type in discs that has received much attention, partly in … planetesimal
formation, are vortices. They can arise in both self-gravitating and non-self-gravitating discs …

… small planetesimals (radii ∼1–10 m) in marginally stable, self-gravitating protoplanetary
discs… how the interaction between a self-gravitating gaseous protoplanetary disc and embedded …

… We investigate the kinematic evolution of planetesimals in self-gravitating discs, combining
… of the disc gas with a gravitationally coupled population of test particle planetesimals. We find …

… discs with some application related to planet formation. In sect. 8 I focus on the impact of
self-gravity in AGN discs also showing how self-gravitating accretion discs … the formation of the …

… In this paper, we simulate the interaction of a gaseous self-gravitating disc with a small
number of planetesimals using SPH, a Lagrangian particle based method (Lucy 1977; Benz 1990…

… of planetesimals together, in a manner which results in mass growth, until a planet is formed.
… orbit surrounded by a self-gravitating disc, the gravitational potential experienced by the …

… Our results for the orbital evolution of protoplanetary cores in self-gravitating discs around
… in the early stages of planet formation, trapping large numbers of planetesimals, boulders or …