589 citations · 3.6k across the 42 of their papers we have counts for
42 papers
On the interaction of pebble accreting embryos with the gaseous disc: importance of thermal forces
S. Cornejo, F. S. Masset, F. J. Sánchez-Salcedo
A planetary embryo embedded in a gaseous disc can grow by pebble accretion while subjected to a gravitational force from the disc that changes its orbital elements. Usually, that f…
Evolution of the eccentricity and inclination of low-mass planets subjected to thermal forces: a numerical study
S. Cornejo, F. S. Masset, R. O. Chametla +1
By means of three dimensional, high resolution hydrodynamical simulations we study the orbital evolution of weakly eccentric or inclined low-mass protoplanets embedded in gaseous d…
Planet-Disk Interactions
Sijme-Jan Paardekooper, Ruobing Dong, Paul Duffell +4
Planet-disk interactions, where an embedded massive body interacts gravitationally with the protoplanetary disk it was formed in, can play an important role in reshaping both the d…
How the planetary eccentricity influences the pebble isolation mass
Raúl O. Chametla, Frédéric S. Masset, Clément Baruteau +1
We investigate the pebble isolation mass for a planet on a fixed eccentric orbit in its protoplanetary disc by conducting a set of 2D hydrodynamical simulations including dust turb…
Eccentricity driving of pebble accreting low-mass planets
David A. Velasco-Romero, Frédéric S. Masset, Romain Teyssier
By means of high resolution hydrodynamical, three-dimensional calculations with nested-meshes, we evaluate the eccentricity reached by a low-mass, luminous planet embedded in an in…
The importance of thermal torques on the migration of planets growing by pebble accretion
O. M. Guilera, M. M. Miller Bertolami, F. Masset +3
A key process in planet formation is the exchange of angular momentum between a growing planet and the protoplanetary disc, which makes the planet migrate through the disc. Several…