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) -
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) -
On some aspects of the stirring rate of planetesimal velocities by a protoplanet
por: Brunini, Adrián, et al.
Publicado: (2007) -
Revealing the parameters of the open cluster Ruprecht 58
por: Giorgi, Edgard Ervar Salvador, et al.
Publicado: (2007)