The Influence of Cold Jupiters in the Formation of Close-in Planets. I. Planetesimal Transport
The formation of a cold Jupiter (CJ) is expected to quench the influx of pebbles and the migration of cores interior to its orbit, thus limiting the efficiency of rocky planet formation either by pebble accretion and/or orbital migration. Observations, however, show that the presence of outer CJs (>...
Guardado en:
| Autores principales: | , , |
|---|---|
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
IOP Publishing
2023-01-01
|
| Colección: | The Astrophysical Journal |
| Materias: | |
| Acceso en línea: | https://doi.org/10.3847/1538-4357/ad0965 |
| Etiquetas: |
Sin Etiquetas, Sea el primero en etiquetar este registro!
|