Core instability models of giant planet accretion and the planetary desert

Miguel, Yamila et al · SEDICI UNLP · 2008

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Miguel, Yamila et al

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SEDICI UNLP

Year

2008

Language

English

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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 consequences that different prescriptions for the solid and gas accretion rates would have on this distribution and found that it is strongly dependent on the adopted model for the gas accretion. Facultad de Ciencias Astronómicas y Geofísicas

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APA 7

Miguel, Y. E. A. (2008). Core instability models of giant planet accretion and the planetary desert. http://sedici.unlp.edu.ar/handle/10915/2093

MLA

Miguel, Yamila et al. "Core instability models of giant planet accretion and the planetary desert." 2008. http://sedici.unlp.edu.ar/handle/10915/2093.

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Miguel, Yamila et al. 2008. "Core instability models of giant planet accretion and the planetary desert.". http://sedici.unlp.edu.ar/handle/10915/2093.

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Miguel, Y. E. A. 2008, Core instability models of giant planet accretion and the planetary desert, SEDICI UNLP, available at: http://sedici.unlp.edu.ar/handle/10915/2093 [Accessed 8 Aug. 2026].

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Title: Core instability models of giant planet accretion and the planetary desert

Author / contributors: Miguel, Yamila et al

Publisher: SEDICI UNLP

Publication year: 2008

Language: English

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Ciencias Astronómicas; planets and satellites; planetología; Sistema Solar; solar system: formation; astrofísica