Envelope instability in giant planet formation

We compute the growth of isolated gaseous giant planets for several values of the density of the protoplanetary disk, several distances from the central star and two values for the (fixed) radii of accreted planetesimals. Calculations were performed in the frame of the core instability mechanism and...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Benvenuto, Omar Gustavo, Brunini, Adrián, Fortier, Andrea
Formato: Articulo
Publicado: 2007
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/2096
Aporte de:

Ejemplares similares