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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 (>...

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Auteurs principaux: Marcy Best, Antranik A. Sefilian, Cristobal Petrovich
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2023-01-01
Collection:The Astrophysical Journal
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Accès en ligne:https://doi.org/10.3847/1538-4357/ad0965
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