Evolution of the eccentricity and inclination of low-mass planets subjected to thermal forces: a numerical study

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 discs subject to thermal diffusion. We consider both non-luminous planets, and planets that also experience the radiative...

Full description

Saved in:
Bibliographic Details
Published inarXiv.org
Main Authors Cornejo, S, Masset, F S, Chametla, R O, Fromenteau, S
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 01.03.2023
Subjects
Online AccessGet full text

Cover

Loading…