The role of the initial surface density profiles of the disc on giant planet formation: comparing with observations
In order to explain the main characteristics of the observed population of extrasolar planets and the giant planets in the Solar system, we need to get a clear understanding of which are the initial conditions that allowed their formation. To this end we develop a semi-analytical model for computing...
Guardado en:
| Autores principales: | Miguel, Yamila, Guilera, Octavio Miguel, Brunini, Adrián |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2011
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84197 |
| Aporte de: |
Ejemplares similares
-
Giant planet formation at the pressure maxima of protoplanetary disks
por: Guilera, Octavio Miguel, et al.
Publicado: (2017) -
Terrestrial-type planet formation : Comparing different types of initial conditions
por: Ronco, María Paula, et al.
Publicado: (2015) -
Core instability models of giant planet accretion and the planetary desert
por: Miguel, Yamila, et al.
Publicado: (2008) -
Planetesimal fragmentation and giant planet formation
por: Guilera, Octavio Miguel, et al.
Publicado: (2014) -
Simultaneous formation of solar system giant planets
por: Guilera, Octavio Miguel, et al.
Publicado: (2011)