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...
Guardado en:
| Autores principales: | Benvenuto, Omar Gustavo, Brunini, Adrián, Fortier, Andrea |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2007
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/2096 http://www.sciencedirect.com/science/article/pii/S0019103507002850 |
| Aporte de: |
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