Core instability models of giant planet accretion : II. Forming planetary systems
We develop a simple model for computing planetary formation based on the core instability model for the gas accretion and the oligarchic growth regime for the accretion of the solid core. In this model several planets can form simultaneously in the disc, a fact that has important implications especi...
Guardado en:
| Autores principales: | Miguel, Yamila, Brunini, Adrián |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2009
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/2091 http://mnras.oxfordjournals.org/content/392/1/391 |
| Aporte de: |
Ejemplares similares
-
Core instability models of giant planet accretion and the planetary desert
por: Miguel, Yamila, et al.
Publicado: (2008) -
Envelope instability in giant planet formation
por: Benvenuto, Omar Gustavo, et al.
Publicado: (2007) -
Oligarchic planetesimal accretion and giant planet formation II
por: Fortier, Andrea, et al.
Publicado: (2009) -
Core instability models of giant planet accretion and the planetary desert
por: Miguel, Yamila, et al.
Publicado: (2008) -
The effects of ablation on the cross section of planetary envelopes at capturing planetesimals
por: Benvenuto, Omar Gustavo, et al.
Publicado: (2008)