La abundancia de galaxias y halos de materia oscura en el universo CDM

Autores
Abadi, Mario Gabriel; Benítez-Llambay, A.; Ferrero, I.
Año de publicación
2013
Idioma
español castellano
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Abstract: We use the GIMIC cosmological hydrodynamical simulations to perform a study of the properties of spheroidal galaxies formed without merger events. We select a sample of galaxies with stellar mass greater than 10 M and we classified them according to the degree of rotation support through the ratio of the rotational kinetic energy respect to the total at redshift z=0. Taken only those with ; we focus on those with accreted mass fraction less than 20 to ensure that they are merger free. We found that these spheroidal galaxies have stellar mass M M and have an important barred component. Interestingly; we found that in many cases the simulated galaxies present two external rings around the bar being both coplanar and counter-rotating to each other. FULL TEXT IN SPANISH
Fil: Abadi, Mario Gabriel. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina.
Fil: Abadi, Mario Gabriel. Conicet. Instituto de Astronomía Teórica y Experimental; Argentina.
http://www.astronomiaargentina.org.ar/uploads/docs/baaa56.pdf
Astronomía (incluye Astrofísica y Ciencias del Espacio)
Materia
Abundancia
Galaxias
Halos
Nivel de accesibilidad
acceso abierto
Condiciones de uso
Repositorio
Repositorio Digital Universitario (UNC)
Institución
Universidad Nacional de Córdoba
OAI Identificador
oai:rdu.unc.edu.ar:11086/18951
Acceder
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network_acronym_str RDUUNC
repository_id_str 2572
network_name_str Repositorio Digital Universitario (UNC)
spelling La abundancia de galaxias y halos de materia oscura en el universo CDMAbadi, Mario GabrielBenítez-Llambay, A.Ferrero, I.AbundanciaGalaxiasHalosAbstract: We use the GIMIC cosmological hydrodynamical simulations to perform a study of the properties of spheroidal galaxies formed without merger events. We select a sample of galaxies with stellar mass greater than 10 M and we classified them according to the degree of rotation support through the ratio of the rotational kinetic energy respect to the total at redshift z=0. Taken only those with ; we focus on those with accreted mass fraction less than 20 to ensure that they are merger free. We found that these spheroidal galaxies have stellar mass M M and have an important barred component. Interestingly; we found that in many cases the simulated galaxies present two external rings around the bar being both coplanar and counter-rotating to each other. FULL TEXT IN SPANISHFil: Abadi, Mario Gabriel. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina.Fil: Abadi, Mario Gabriel. Conicet. Instituto de Astronomía Teórica y Experimental; Argentina.http://www.astronomiaargentina.org.ar/uploads/docs/baaa56.pdfAstronomía (incluye Astrofísica y Ciencias del Espacio)Tandil2013info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttp://hdl.handle.net/11086/18951https://ui.adsabs.harvard.edu/abs/2013BAAA...56...33A/abstractspainfo:eu-repo/semantics/openAccessreponame:Repositorio Digital Universitario (UNC)instname:Universidad Nacional de Córdobainstacron:UNC2025-10-16T09:30:58Zoai:rdu.unc.edu.ar:11086/18951Institucionalhttps://rdu.unc.edu.ar/Universidad públicaNo correspondehttp://rdu.unc.edu.ar/oai/snrdoca.unc@gmail.comArgentinaNo correspondeNo correspondeNo correspondeopendoar:25722025-10-16 09:30:58.476Repositorio Digital Universitario (UNC) - Universidad Nacional de Córdobafalse
dc.title.none.fl_str_mv La abundancia de galaxias y halos de materia oscura en el universo CDM
title La abundancia de galaxias y halos de materia oscura en el universo CDM
spellingShingle La abundancia de galaxias y halos de materia oscura en el universo CDM
Abadi, Mario Gabriel
Abundancia
Galaxias
Halos
title_short La abundancia de galaxias y halos de materia oscura en el universo CDM
title_full La abundancia de galaxias y halos de materia oscura en el universo CDM
title_fullStr La abundancia de galaxias y halos de materia oscura en el universo CDM
title_full_unstemmed La abundancia de galaxias y halos de materia oscura en el universo CDM
title_sort La abundancia de galaxias y halos de materia oscura en el universo CDM
dc.creator.none.fl_str_mv Abadi, Mario Gabriel
Benítez-Llambay, A.
Ferrero, I.
author Abadi, Mario Gabriel
author_facet Abadi, Mario Gabriel
Benítez-Llambay, A.
Ferrero, I.
author_role author
author2 Benítez-Llambay, A.
Ferrero, I.
author2_role author
author
dc.subject.none.fl_str_mv Abundancia
Galaxias
Halos
topic Abundancia
Galaxias
Halos
dc.description.none.fl_txt_mv Abstract: We use the GIMIC cosmological hydrodynamical simulations to perform a study of the properties of spheroidal galaxies formed without merger events. We select a sample of galaxies with stellar mass greater than 10 M and we classified them according to the degree of rotation support through the ratio of the rotational kinetic energy respect to the total at redshift z=0. Taken only those with ; we focus on those with accreted mass fraction less than 20 to ensure that they are merger free. We found that these spheroidal galaxies have stellar mass M M and have an important barred component. Interestingly; we found that in many cases the simulated galaxies present two external rings around the bar being both coplanar and counter-rotating to each other. FULL TEXT IN SPANISH
Fil: Abadi, Mario Gabriel. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina.
Fil: Abadi, Mario Gabriel. Conicet. Instituto de Astronomía Teórica y Experimental; Argentina.
http://www.astronomiaargentina.org.ar/uploads/docs/baaa56.pdf
Astronomía (incluye Astrofísica y Ciencias del Espacio)
description Abstract: We use the GIMIC cosmological hydrodynamical simulations to perform a study of the properties of spheroidal galaxies formed without merger events. We select a sample of galaxies with stellar mass greater than 10 M and we classified them according to the degree of rotation support through the ratio of the rotational kinetic energy respect to the total at redshift z=0. Taken only those with ; we focus on those with accreted mass fraction less than 20 to ensure that they are merger free. We found that these spheroidal galaxies have stellar mass M M and have an important barred component. Interestingly; we found that in many cases the simulated galaxies present two external rings around the bar being both coplanar and counter-rotating to each other. FULL TEXT IN SPANISH
publishDate 2013
dc.date.none.fl_str_mv 2013
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11086/18951
https://ui.adsabs.harvard.edu/abs/2013BAAA...56...33A/abstract
url http://hdl.handle.net/11086/18951
https://ui.adsabs.harvard.edu/abs/2013BAAA...56...33A/abstract
dc.language.none.fl_str_mv spa
language spa
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Tandil
publisher.none.fl_str_mv Tandil
dc.source.none.fl_str_mv reponame:Repositorio Digital Universitario (UNC)
instname:Universidad Nacional de Córdoba
instacron:UNC
reponame_str Repositorio Digital Universitario (UNC)
collection Repositorio Digital Universitario (UNC)
instname_str Universidad Nacional de Córdoba
instacron_str UNC
institution UNC
repository.name.fl_str_mv Repositorio Digital Universitario (UNC) - Universidad Nacional de Córdoba
repository.mail.fl_str_mv oca.unc@gmail.com
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score 12.712165

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