Stellar irradiated discs and implications on migration of embedded planets

2012/11/15 by B. Bitsch, Bertram Bitsch, A. Crida +7 · 2 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Hot Jupiter #Irradiation #Low Mass #Planet #Planetary mass #Planetary system #Radiative equilibrium #Radiative transfer #Stellar, planetary, and galactic studies #astro-ph.EP

paper · pdf · doi:10.1051/0004-6361/201220159

openalex publication_date 2012/11/15 · arxiv created 2012/12/02 · arxiv updated 2014/01/09 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The strength and direction of migration of embedded low mass planets depends on the disc’s thermodynamic state. It has been shown that, in discs where the viscous heating is balanced by radiative transport, the migration can be directed outwards, a process which extends the lifetime of growing planetary embryos.

Citations

• Cavity opening by a giant planet in a protoplanetary disc and effects on planetary migration
• Passive Irradiated Circumstellar Disks with an Inner Hole
• SATURATED TORQUE FORMULA FOR PLANETARY MIGRATION IN VISCOUS DISKS WITH THERMAL DIFFUSION: RECIPE FOR PROTOPLANET POPULATION SYNTHESIS
• The distribution of mass in the planetary system and solar nebula
• RADIATIVE HYDRODYNAMIC SIMULATIONS OF HD209458b: TEMPORAL VARIABILITY
• Using FU Orionis outbursts to constrain self-regulated protostellar disk models
• Halting type I planet migration in non-isothermal disks
• On disc protoplanet interactions in a non-barotropic disc with thermal diffusion
• Rosseland and Planck mean opacities for protoplanetary discs

Cited by

• Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall
• Formation of planetary systems by pebble accretion and migration: Hot super-Earth systems from breaking compact resonant chains