Planetesimal fragmentation and giant planet formation

Context. In the standard scenario of planet formation, terrestrial planets and the cores of the giant planets are formed by accretion of planetesimals. As planetary embryos grow, the planetesimal velocity dispersion increases because of gravitational excitations produced by embryos. The increasing r...

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Detalles Bibliográficos
Autores principales:	Guilera, Octavio Miguel, Elía, Gonzalo Carlos de, Brunini, Adrián, Santamaría, Pablo Javier
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2014
Materias:	Ciencias Astronómicas Methods: numerical Planets and satellites: formation
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85557
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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