Giant planet formation at the pressure maxima of protoplanetary disks

Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accretion timescales of kilometer size planetesimals may not favor the formation of massive cores of giant planets before the dissipation of protoplanetary disks. On the other hand, the existence of pressu...

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Detalles Bibliográficos
Autores principales:	Guilera, Octavio Miguel, Sándor, Zs
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2017
Materias:	Ciencias Astronómicas Planets and satellites: Formation Planets and satellites: Gaseous planets Protoplanetary disks
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/87247
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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