Core instability models of giant planet accretion and the planetary desert
- Autores
- Miguel, Yamila; Brunini, Adrián
- Año de publicación
- 2008
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
Planets and satellites: formation
Solar system: formation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/123810
Ver los metadatos del registro completo
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Core instability models of giant planet accretion and the planetary desertMiguel, YamilaBrunini, AdriánCiencias AstronómicasPlanets and satellites: formationSolar system: formationWith 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 GeofísicasInstituto de Astrofísica de La Plata2008info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf463-468http://sedici.unlp.edu.ar/handle/10915/123810enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/issn/1365-2966info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13261.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:10:24Zoai:sedici.unlp.edu.ar:10915/123810Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:10:24.478SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Core instability models of giant planet accretion and the planetary desert |
| title |
Core instability models of giant planet accretion and the planetary desert |
| spellingShingle |
Core instability models of giant planet accretion and the planetary desert Miguel, Yamila Ciencias Astronómicas Planets and satellites: formation Solar system: formation |
| title_short |
Core instability models of giant planet accretion and the planetary desert |
| title_full |
Core instability models of giant planet accretion and the planetary desert |
| title_fullStr |
Core instability models of giant planet accretion and the planetary desert |
| title_full_unstemmed |
Core instability models of giant planet accretion and the planetary desert |
| title_sort |
Core instability models of giant planet accretion and the planetary desert |
| dc.creator.none.fl_str_mv |
Miguel, Yamila Brunini, Adrián |
| author |
Miguel, Yamila |
| author_facet |
Miguel, Yamila Brunini, Adrián |
| author_role |
author |
| author2 |
Brunini, Adrián |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Planets and satellites: formation Solar system: formation |
| topic |
Ciencias Astronómicas Planets and satellites: formation Solar system: formation |
| dc.description.none.fl_txt_mv |
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 Instituto de Astrofísica de La Plata |
| description |
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. |
| publishDate |
2008 |
| dc.date.none.fl_str_mv |
2008 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/123810 |
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| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/issn/1365-2966 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13261.x |
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openAccess |
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