124 citations · 520 across the 19 of their papers we have counts for
16 papers · 1 filter
A recipe for eccentricity and inclination damping for partial gap opening planets in 3D disks
Gabriele Pichierri, Bertram Bitsch, Elena Lega
In a previous paper we showed that, like the migration speed, the eccentricity damping efficiency is modulated linearly by the depth of the partial gap a planet carves in the disk…
Which stars can form planets: Planetesimal formation at low metallicities
Geoffrey Andama, Jingyi Mah, Bertram Bitsch
The exoplanet diversity has been linked to the disc environment in which they form, where the host star metallicity and the formation pathways play a crucial role. In the context o…
Composition of giant planets: the roles of pebbles and planetesimals
Claudia Danti, Bertram Bitsch, Jingyi Mah
One of the current challenges of planet formation theory is to explain the enrichment of observed exoplanetary atmospheres. Past studies have focused on scenarios where either pebb…
Enriching inner discs and giant planets with heavy elements
Bertram Bitsch, Jingyi Mah
Giant exoplanets seem to have on average a much larger heavy element content than the solar system giants. Past attempts to explain these heavy element contents include collisions…
How to make giant planets via pebble accretion
Sofia Savvidou, Bertram Bitsch
Planet formation is directly linked to the birthing environment that protoplanetary disks provide. The disk properties determine whether a giant planet will form and how it evolves…
Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars
J. Mah, B. Bitsch, I. Pascucci +1
The origin of the elevated C/O ratios in discs around late M dwarfs compared to discs around solar-type stars is not well understood. Here we endeavour to reproduce the observed di…