Core instability models of giant planet accretion and the planetary desert
With the aim of studying the final mass distribution of extrasolar planets, we have developed a simple model based on the core instability model, which allows us to form a large population of planets and make them evolve in circumstellar discs with various initial conditions. We investigate the cons...
Guardado en:
| Autores principales: | Miguel, Yamila, Brunini, Adrián |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2008
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/2093 http://mnras.oxfordjournals.org/content/387/1/463 |
| Aporte de: |
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