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
Materia
Ciencias Astronómicas
planets and satellites
planetología
Sistema Solar
solar system: formation
astrofísica
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-nd/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/2093
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/2093
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Core instability models of giant planet accretion and the planetary desertMiguel, YamilaBrunini, AdriánCiencias Astronómicasplanets and satellitesplanetologíaSistema Solarsolar system: formationastrofísicaWith 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 Geofísicas2008info: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/10915/2093enginfo:eu-repo/semantics/altIdentifier/url/http://mnras.oxfordjournals.org/content/387/1/463info: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-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T10:48:37Zoai:sedici.unlp.edu.ar:10915/2093Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 10:48:39.111SEDICI (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
planetología
Sistema Solar
solar system: formation
astrofísica
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
planetología
Sistema Solar
solar system: formation
astrofísica
topic Ciencias Astronómicas
planets and satellites
planetología
Sistema Solar
solar system: formation
astrofísica
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
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
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/2093
url http://sedici.unlp.edu.ar/handle/10915/2093
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://mnras.oxfordjournals.org/content/387/1/463
info:eu-repo/semantics/altIdentifier/issn/1365-2966
info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13261.x
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-nd/4.0/
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-nd/4.0/
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
dc.format.none.fl_str_mv application/pdf
463-468
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.070432

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