Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation
- Autores
- Tissera, Patricia Beatriz; de Rossi, Maria Emilia; Scannapieco, Cecilia
- Año de publicación
- 2005
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We study the mass–metallicity relation of galactic systems with stellar masses larger than 109M⊙h−1 in Λ cold dark matter scenarios by using chemical hydrodynamical simulations. We find that this relation arises naturally as a consequence of the formation of the structure in a hierarchical scenario. The hierarchical building-up of the structure determines a characteristic stellar mass at Mc≈ 1010.2M⊙h−1 which exhibits approximately solar metallicities from z≈ 3 to z= 0. This characteristic mass separates galactic systems into two groups with massive ones forming most of their stars and metals at high redshift. We find evolution in the zero point and slope of the mass–metallicity relation driven mainly by the low-mass systems which exhibit the larger variations in the chemical properties. Although stellar mass and circular velocity are directly related, the correlation between circular velocity and metallicity shows a larger evolution with redshift because of the combination of chemical evolution and cosmology. The dispersion found in both relations is a function of the stellar mass and reflects the different dynamical history of evolution of the systems.
Fil: Tissera, Patricia Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: de Rossi, Maria Emilia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Scannapieco, Cecilia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina - Materia
-
METHODS:NUMERICAL
GALAXIES:ABUNDANCES
GALAXIES:EVOLUTION
GALAXIES;FORMATION
COSMOLOGY:THEORY - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/22047
Ver los metadatos del registro completo
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Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relationTissera, Patricia Beatrizde Rossi, Maria EmiliaScannapieco, CeciliaMETHODS:NUMERICALGALAXIES:ABUNDANCESGALAXIES:EVOLUTIONGALAXIES;FORMATIONCOSMOLOGY:THEORYhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study the mass–metallicity relation of galactic systems with stellar masses larger than 109M⊙h−1 in Λ cold dark matter scenarios by using chemical hydrodynamical simulations. We find that this relation arises naturally as a consequence of the formation of the structure in a hierarchical scenario. The hierarchical building-up of the structure determines a characteristic stellar mass at Mc≈ 1010.2M⊙h−1 which exhibits approximately solar metallicities from z≈ 3 to z= 0. This characteristic mass separates galactic systems into two groups with massive ones forming most of their stars and metals at high redshift. We find evolution in the zero point and slope of the mass–metallicity relation driven mainly by the low-mass systems which exhibit the larger variations in the chemical properties. Although stellar mass and circular velocity are directly related, the correlation between circular velocity and metallicity shows a larger evolution with redshift because of the combination of chemical evolution and cosmology. The dispersion found in both relations is a function of the stellar mass and reflects the different dynamical history of evolution of the systems.Fil: Tissera, Patricia Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: de Rossi, Maria Emilia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Scannapieco, Cecilia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaOxford University Press2005-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/22047Tissera, Patricia Beatriz; de Rossi, Maria Emilia; Scannapieco, Cecilia; Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 364; 1; 12-2005; L38-L410035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2005.00101.xinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnrasl/article-lookup/doi/10.1111/j.1745-3933.2005.00101.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:58:32Zoai:ri.conicet.gov.ar:11336/22047instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:58:32.807CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation |
title |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation |
spellingShingle |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation Tissera, Patricia Beatriz METHODS:NUMERICAL GALAXIES:ABUNDANCES GALAXIES:EVOLUTION GALAXIES;FORMATION COSMOLOGY:THEORY |
title_short |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation |
title_full |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation |
title_fullStr |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation |
title_full_unstemmed |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation |
title_sort |
Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation |
dc.creator.none.fl_str_mv |
Tissera, Patricia Beatriz de Rossi, Maria Emilia Scannapieco, Cecilia |
author |
Tissera, Patricia Beatriz |
author_facet |
Tissera, Patricia Beatriz de Rossi, Maria Emilia Scannapieco, Cecilia |
author_role |
author |
author2 |
de Rossi, Maria Emilia Scannapieco, Cecilia |
author2_role |
author author |
dc.subject.none.fl_str_mv |
METHODS:NUMERICAL GALAXIES:ABUNDANCES GALAXIES:EVOLUTION GALAXIES;FORMATION COSMOLOGY:THEORY |
topic |
METHODS:NUMERICAL GALAXIES:ABUNDANCES GALAXIES:EVOLUTION GALAXIES;FORMATION COSMOLOGY:THEORY |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We study the mass–metallicity relation of galactic systems with stellar masses larger than 109M⊙h−1 in Λ cold dark matter scenarios by using chemical hydrodynamical simulations. We find that this relation arises naturally as a consequence of the formation of the structure in a hierarchical scenario. The hierarchical building-up of the structure determines a characteristic stellar mass at Mc≈ 1010.2M⊙h−1 which exhibits approximately solar metallicities from z≈ 3 to z= 0. This characteristic mass separates galactic systems into two groups with massive ones forming most of their stars and metals at high redshift. We find evolution in the zero point and slope of the mass–metallicity relation driven mainly by the low-mass systems which exhibit the larger variations in the chemical properties. Although stellar mass and circular velocity are directly related, the correlation between circular velocity and metallicity shows a larger evolution with redshift because of the combination of chemical evolution and cosmology. The dispersion found in both relations is a function of the stellar mass and reflects the different dynamical history of evolution of the systems. Fil: Tissera, Patricia Beatriz. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: de Rossi, Maria Emilia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Scannapieco, Cecilia. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina |
description |
We study the mass–metallicity relation of galactic systems with stellar masses larger than 109M⊙h−1 in Λ cold dark matter scenarios by using chemical hydrodynamical simulations. We find that this relation arises naturally as a consequence of the formation of the structure in a hierarchical scenario. The hierarchical building-up of the structure determines a characteristic stellar mass at Mc≈ 1010.2M⊙h−1 which exhibits approximately solar metallicities from z≈ 3 to z= 0. This characteristic mass separates galactic systems into two groups with massive ones forming most of their stars and metals at high redshift. We find evolution in the zero point and slope of the mass–metallicity relation driven mainly by the low-mass systems which exhibit the larger variations in the chemical properties. Although stellar mass and circular velocity are directly related, the correlation between circular velocity and metallicity shows a larger evolution with redshift because of the combination of chemical evolution and cosmology. The dispersion found in both relations is a function of the stellar mass and reflects the different dynamical history of evolution of the systems. |
publishDate |
2005 |
dc.date.none.fl_str_mv |
2005-12 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://hdl.handle.net/11336/22047 Tissera, Patricia Beatriz; de Rossi, Maria Emilia; Scannapieco, Cecilia; Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 364; 1; 12-2005; L38-L41 0035-8711 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/22047 |
identifier_str_mv |
Tissera, Patricia Beatriz; de Rossi, Maria Emilia; Scannapieco, Cecilia; Fingerprints of the hierarchical building-up of the structure on the mass-metallicity relation; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 364; 1; 12-2005; L38-L41 0035-8711 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1745-3933.2005.00101.x info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnrasl/article-lookup/doi/10.1111/j.1745-3933.2005.00101.x |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Oxford University Press |
publisher.none.fl_str_mv |
Oxford University Press |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613743922642944 |
score |
13.070432 |