Outer-disk reddening and gas-phase metallicities: The CALIFA connection

Autores
Marino, R. A.; Gil de Paz, A.; Sánchez, S. F.; Sanchez Blazquez, P.; Cardiel, N.; Castillo Morales, A.; Pascual, S.; Vilchez, J.; Kehrig, C.; Mollá, M.; Mendez-Abreu, J.; Catalán Torrecilla, C.; Florido, E; Pérez, I.; Ruiz-Lara, T; Ellis, S.; López-Sánchez, A. R.; González Delgado, R. M.; de Lorenzo-Cáceres, A.; García Benito, R.; Galbany, L.; Zibetti, S.; Cortijo, C.; Kalinova, V; Mast, Damian; Iglesias Páramo, J.; Papaderos, P.; Walcher, C. J.; Bland Hawthorn, J.; The CALIFA Team
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We study, for the first time in a statistically significant and well-defined sample, the relation between the outer-disk ionized-gas metallicity gradients and the presence of breaks in the surface brightness profiles of disk galaxies. Sloan Digital Sky Survey (SDSS) g′- and r′-band surface brightness, (g′ - r′) color, and ionized-gas oxygen abundance profiles for 324 galaxies within the Calar Alto Legacy Integral Field Area (CALIFA) survey are used for this purpose. We perform a detailed light-profile classification, finding that 84% of our disks show down- or up-bending profiles (Type II and Type III, respectively), while the remaining 16% are well fitted by one single exponential (Type I). The analysis of the color gradients at both sides of this break shows a U-shaped profile for most Type II galaxies with an average minimum (g′ - r′) color of ∼ 0.5mag and an ionized-gas metallicity flattening associated with it only in the case of low-mass galaxies. Comparatively, more massive systems show a rather uniform negative metallicity gradient. The correlation between metallicity flattening and stellar mass for these systems results in p-values as low as 0.01. Independent of the mechanism having shaped the outer light profiles of these galaxies, stellar migration or a previous episode of star formation in a shrinking star-forming disk, it is clear that the imprint in their ionized-gas metallicity was different for low- and high-mass Type II galaxies. In the case of Type III disks, a positive correlation between the change in color and abundance gradient is found (the null hypothesis is ruled out with a p-value of 0.02), with the outer disks of Type III galaxies with masses ≤1010 M′ showing a weak color reddening or even a bluing. This is interpreted as primarily due to a mass downsizing effect on the population of Type III galaxies that recently experienced an enhanced inside-out growth.
Fil: Marino, R. A.. Universidad Complutense de Madrid; España. Institute for Astronomy; Suiza
Fil: Gil de Paz, A.. Universidad Complutense de Madrid; España
Fil: Sánchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Fil: Sanchez Blazquez, P.. Universidad Autónoma de Madrid; España
Fil: Cardiel, N.. Universidad Complutense de Madrid; España. Instituto de Física de Cantabria; España
Fil: Castillo Morales, A.. Universidad Complutense de Madrid; España
Fil: Pascual, S.. Universidad Complutense de Madrid; España
Fil: Vilchez, J.. Instituto de Astrofísica de Andalucía; España
Fil: Kehrig, C.. Instituto de Astrofísica de Andalucía; España
Fil: Mollá, M.. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; España
Fil: Mendez-Abreu, J.. University of St. Andrews; Reino Unido
Fil: Catalán Torrecilla, C.. Universidad Complutense de Madrid; España
Fil: Florido, E. Universidad de Granada. Facultad de Ciencias; España
Fil: Pérez, I.. Universidad de Granada. Facultad de Ciencias; España
Fil: Ruiz-Lara, T. Universidad de Granada. Facultad de Ciencias; España
Fil: Ellis, S.. Australian Astronomical Observatory; Australia
Fil: López-Sánchez, A. R.. Australian Astronomical Observatory; Australia. Macquarie University; Australia
Fil: González Delgado, R. M.. Instituto de Astrofísica de Andalucía; España
Fil: de Lorenzo-Cáceres, A.. University of St. Andrews; Reino Unido
Fil: García Benito, R.. Instituto de Astrofísica de Andalucía; España
Fil: Galbany, L.. Millennium Institute Of Astrophysics, Chile; Chile. Universidad de Chile; Chile
Fil: Zibetti, S.. Osservatorio Astrofisico di Arcetri; Italia
Fil: Cortijo, C.. Instituto de Astrofísica de Andalucía; España
Fil: Kalinova, V. University of Alberta; Canadá
Fil: Mast, Damian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Centro Brasileiro de Pesquisas Físicas; Brasil
Fil: Iglesias Páramo, J.. Instituto de Astrofísica de Andalucía; España. Consejo Superior de Investigaciones Científicas. Estación Experimental de Zonas Aridas; España
Fil: Papaderos, P.. Universidad de Porto; Portugal
Fil: Walcher, C. J.. Leibniz-Institut für Astrophysik Potsdam; Alemania
Fil: Bland Hawthorn, J.. Sydney Institute For Astronomy; Australia
Fil: The CALIFA Team. Consejo Superior de Investigaciones Científicas. Estación Experimental de Zonas Aridas; España
Materia
GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: ISM
GALAXIES: PHOTOMETRY
HII REGIONS
ISM: ABUNDANCES
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/78746

id CONICETDig_6a9ecb5b8884d13686d0327aff2c4819
oai_identifier_str oai:ri.conicet.gov.ar:11336/78746
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Outer-disk reddening and gas-phase metallicities: The CALIFA connectionMarino, R. A.Gil de Paz, A.Sánchez, S. F.Sanchez Blazquez, P.Cardiel, N.Castillo Morales, A.Pascual, S.Vilchez, J.Kehrig, C.Mollá, M.Mendez-Abreu, J.Catalán Torrecilla, C.Florido, EPérez, I.Ruiz-Lara, TEllis, S.López-Sánchez, A. R.González Delgado, R. M.de Lorenzo-Cáceres, A.García Benito, R.Galbany, L.Zibetti, S.Cortijo, C.Kalinova, VMast, DamianIglesias Páramo, J.Papaderos, P.Walcher, C. J.Bland Hawthorn, J.The CALIFA TeamGALAXIES: ABUNDANCESGALAXIES: EVOLUTIONGALAXIES: ISMGALAXIES: PHOTOMETRYHII REGIONSISM: ABUNDANCEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We study, for the first time in a statistically significant and well-defined sample, the relation between the outer-disk ionized-gas metallicity gradients and the presence of breaks in the surface brightness profiles of disk galaxies. Sloan Digital Sky Survey (SDSS) g′- and r′-band surface brightness, (g′ - r′) color, and ionized-gas oxygen abundance profiles for 324 galaxies within the Calar Alto Legacy Integral Field Area (CALIFA) survey are used for this purpose. We perform a detailed light-profile classification, finding that 84% of our disks show down- or up-bending profiles (Type II and Type III, respectively), while the remaining 16% are well fitted by one single exponential (Type I). The analysis of the color gradients at both sides of this break shows a U-shaped profile for most Type II galaxies with an average minimum (g′ - r′) color of ∼ 0.5mag and an ionized-gas metallicity flattening associated with it only in the case of low-mass galaxies. Comparatively, more massive systems show a rather uniform negative metallicity gradient. The correlation between metallicity flattening and stellar mass for these systems results in p-values as low as 0.01. Independent of the mechanism having shaped the outer light profiles of these galaxies, stellar migration or a previous episode of star formation in a shrinking star-forming disk, it is clear that the imprint in their ionized-gas metallicity was different for low- and high-mass Type II galaxies. In the case of Type III disks, a positive correlation between the change in color and abundance gradient is found (the null hypothesis is ruled out with a p-value of 0.02), with the outer disks of Type III galaxies with masses ≤1010 M′ showing a weak color reddening or even a bluing. This is interpreted as primarily due to a mass downsizing effect on the population of Type III galaxies that recently experienced an enhanced inside-out growth.Fil: Marino, R. A.. Universidad Complutense de Madrid; España. Institute for Astronomy; SuizaFil: Gil de Paz, A.. Universidad Complutense de Madrid; EspañaFil: Sánchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; MéxicoFil: Sanchez Blazquez, P.. Universidad Autónoma de Madrid; EspañaFil: Cardiel, N.. Universidad Complutense de Madrid; España. Instituto de Física de Cantabria; EspañaFil: Castillo Morales, A.. Universidad Complutense de Madrid; EspañaFil: Pascual, S.. Universidad Complutense de Madrid; EspañaFil: Vilchez, J.. Instituto de Astrofísica de Andalucía; EspañaFil: Kehrig, C.. Instituto de Astrofísica de Andalucía; EspañaFil: Mollá, M.. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; EspañaFil: Mendez-Abreu, J.. University of St. Andrews; Reino UnidoFil: Catalán Torrecilla, C.. Universidad Complutense de Madrid; EspañaFil: Florido, E. Universidad de Granada. Facultad de Ciencias; EspañaFil: Pérez, I.. Universidad de Granada. Facultad de Ciencias; EspañaFil: Ruiz-Lara, T. Universidad de Granada. Facultad de Ciencias; EspañaFil: Ellis, S.. Australian Astronomical Observatory; AustraliaFil: López-Sánchez, A. R.. Australian Astronomical Observatory; Australia. Macquarie University; AustraliaFil: González Delgado, R. M.. Instituto de Astrofísica de Andalucía; EspañaFil: de Lorenzo-Cáceres, A.. University of St. Andrews; Reino UnidoFil: García Benito, R.. Instituto de Astrofísica de Andalucía; EspañaFil: Galbany, L.. Millennium Institute Of Astrophysics, Chile; Chile. Universidad de Chile; ChileFil: Zibetti, S.. Osservatorio Astrofisico di Arcetri; ItaliaFil: Cortijo, C.. Instituto de Astrofísica de Andalucía; EspañaFil: Kalinova, V. University of Alberta; CanadáFil: Mast, Damian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Centro Brasileiro de Pesquisas Físicas; BrasilFil: Iglesias Páramo, J.. Instituto de Astrofísica de Andalucía; España. Consejo Superior de Investigaciones Científicas. Estación Experimental de Zonas Aridas; EspañaFil: Papaderos, P.. Universidad de Porto; PortugalFil: Walcher, C. J.. Leibniz-Institut für Astrophysik Potsdam; AlemaniaFil: Bland Hawthorn, J.. Sydney Institute For Astronomy; AustraliaFil: The CALIFA Team. Consejo Superior de Investigaciones Científicas. Estación Experimental de Zonas Aridas; EspañaEDP Sciences2016-01-16info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/78746Marino, R. A.; Gil de Paz, A.; Sánchez, S. F.; Sanchez Blazquez, P.; Cardiel, N.; et al.; Outer-disk reddening and gas-phase metallicities: The CALIFA connection; EDP Sciences; Astronomy and Astrophysics; 585; 16-1-2016; 1-290004-63611432-0746CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201526986info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2016/01/aa26986-15/aa26986-15.htmlinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:58:05Zoai:ri.conicet.gov.ar:11336/78746instacron: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 09:58:05.552CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Outer-disk reddening and gas-phase metallicities: The CALIFA connection
title Outer-disk reddening and gas-phase metallicities: The CALIFA connection
spellingShingle Outer-disk reddening and gas-phase metallicities: The CALIFA connection
Marino, R. A.
GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: ISM
GALAXIES: PHOTOMETRY
HII REGIONS
ISM: ABUNDANCES
title_short Outer-disk reddening and gas-phase metallicities: The CALIFA connection
title_full Outer-disk reddening and gas-phase metallicities: The CALIFA connection
title_fullStr Outer-disk reddening and gas-phase metallicities: The CALIFA connection
title_full_unstemmed Outer-disk reddening and gas-phase metallicities: The CALIFA connection
title_sort Outer-disk reddening and gas-phase metallicities: The CALIFA connection
dc.creator.none.fl_str_mv Marino, R. A.
Gil de Paz, A.
Sánchez, S. F.
Sanchez Blazquez, P.
Cardiel, N.
Castillo Morales, A.
Pascual, S.
Vilchez, J.
Kehrig, C.
Mollá, M.
Mendez-Abreu, J.
Catalán Torrecilla, C.
Florido, E
Pérez, I.
Ruiz-Lara, T
Ellis, S.
López-Sánchez, A. R.
González Delgado, R. M.
de Lorenzo-Cáceres, A.
García Benito, R.
Galbany, L.
Zibetti, S.
Cortijo, C.
Kalinova, V
Mast, Damian
Iglesias Páramo, J.
Papaderos, P.
Walcher, C. J.
Bland Hawthorn, J.
The CALIFA Team
author Marino, R. A.
author_facet Marino, R. A.
Gil de Paz, A.
Sánchez, S. F.
Sanchez Blazquez, P.
Cardiel, N.
Castillo Morales, A.
Pascual, S.
Vilchez, J.
Kehrig, C.
Mollá, M.
Mendez-Abreu, J.
Catalán Torrecilla, C.
Florido, E
Pérez, I.
Ruiz-Lara, T
Ellis, S.
López-Sánchez, A. R.
González Delgado, R. M.
de Lorenzo-Cáceres, A.
García Benito, R.
Galbany, L.
Zibetti, S.
Cortijo, C.
Kalinova, V
Mast, Damian
Iglesias Páramo, J.
Papaderos, P.
Walcher, C. J.
Bland Hawthorn, J.
The CALIFA Team
author_role author
author2 Gil de Paz, A.
Sánchez, S. F.
Sanchez Blazquez, P.
Cardiel, N.
Castillo Morales, A.
Pascual, S.
Vilchez, J.
Kehrig, C.
Mollá, M.
Mendez-Abreu, J.
Catalán Torrecilla, C.
Florido, E
Pérez, I.
Ruiz-Lara, T
Ellis, S.
López-Sánchez, A. R.
González Delgado, R. M.
de Lorenzo-Cáceres, A.
García Benito, R.
Galbany, L.
Zibetti, S.
Cortijo, C.
Kalinova, V
Mast, Damian
Iglesias Páramo, J.
Papaderos, P.
Walcher, C. J.
Bland Hawthorn, J.
The CALIFA Team
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: ISM
GALAXIES: PHOTOMETRY
HII REGIONS
ISM: ABUNDANCES
topic GALAXIES: ABUNDANCES
GALAXIES: EVOLUTION
GALAXIES: ISM
GALAXIES: PHOTOMETRY
HII REGIONS
ISM: ABUNDANCES
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, for the first time in a statistically significant and well-defined sample, the relation between the outer-disk ionized-gas metallicity gradients and the presence of breaks in the surface brightness profiles of disk galaxies. Sloan Digital Sky Survey (SDSS) g′- and r′-band surface brightness, (g′ - r′) color, and ionized-gas oxygen abundance profiles for 324 galaxies within the Calar Alto Legacy Integral Field Area (CALIFA) survey are used for this purpose. We perform a detailed light-profile classification, finding that 84% of our disks show down- or up-bending profiles (Type II and Type III, respectively), while the remaining 16% are well fitted by one single exponential (Type I). The analysis of the color gradients at both sides of this break shows a U-shaped profile for most Type II galaxies with an average minimum (g′ - r′) color of ∼ 0.5mag and an ionized-gas metallicity flattening associated with it only in the case of low-mass galaxies. Comparatively, more massive systems show a rather uniform negative metallicity gradient. The correlation between metallicity flattening and stellar mass for these systems results in p-values as low as 0.01. Independent of the mechanism having shaped the outer light profiles of these galaxies, stellar migration or a previous episode of star formation in a shrinking star-forming disk, it is clear that the imprint in their ionized-gas metallicity was different for low- and high-mass Type II galaxies. In the case of Type III disks, a positive correlation between the change in color and abundance gradient is found (the null hypothesis is ruled out with a p-value of 0.02), with the outer disks of Type III galaxies with masses ≤1010 M′ showing a weak color reddening or even a bluing. This is interpreted as primarily due to a mass downsizing effect on the population of Type III galaxies that recently experienced an enhanced inside-out growth.
Fil: Marino, R. A.. Universidad Complutense de Madrid; España. Institute for Astronomy; Suiza
Fil: Gil de Paz, A.. Universidad Complutense de Madrid; España
Fil: Sánchez, S. F.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Fil: Sanchez Blazquez, P.. Universidad Autónoma de Madrid; España
Fil: Cardiel, N.. Universidad Complutense de Madrid; España. Instituto de Física de Cantabria; España
Fil: Castillo Morales, A.. Universidad Complutense de Madrid; España
Fil: Pascual, S.. Universidad Complutense de Madrid; España
Fil: Vilchez, J.. Instituto de Astrofísica de Andalucía; España
Fil: Kehrig, C.. Instituto de Astrofísica de Andalucía; España
Fil: Mollá, M.. Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; España
Fil: Mendez-Abreu, J.. University of St. Andrews; Reino Unido
Fil: Catalán Torrecilla, C.. Universidad Complutense de Madrid; España
Fil: Florido, E. Universidad de Granada. Facultad de Ciencias; España
Fil: Pérez, I.. Universidad de Granada. Facultad de Ciencias; España
Fil: Ruiz-Lara, T. Universidad de Granada. Facultad de Ciencias; España
Fil: Ellis, S.. Australian Astronomical Observatory; Australia
Fil: López-Sánchez, A. R.. Australian Astronomical Observatory; Australia. Macquarie University; Australia
Fil: González Delgado, R. M.. Instituto de Astrofísica de Andalucía; España
Fil: de Lorenzo-Cáceres, A.. University of St. Andrews; Reino Unido
Fil: García Benito, R.. Instituto de Astrofísica de Andalucía; España
Fil: Galbany, L.. Millennium Institute Of Astrophysics, Chile; Chile. Universidad de Chile; Chile
Fil: Zibetti, S.. Osservatorio Astrofisico di Arcetri; Italia
Fil: Cortijo, C.. Instituto de Astrofísica de Andalucía; España
Fil: Kalinova, V. University of Alberta; Canadá
Fil: Mast, Damian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Centro Brasileiro de Pesquisas Físicas; Brasil
Fil: Iglesias Páramo, J.. Instituto de Astrofísica de Andalucía; España. Consejo Superior de Investigaciones Científicas. Estación Experimental de Zonas Aridas; España
Fil: Papaderos, P.. Universidad de Porto; Portugal
Fil: Walcher, C. J.. Leibniz-Institut für Astrophysik Potsdam; Alemania
Fil: Bland Hawthorn, J.. Sydney Institute For Astronomy; Australia
Fil: The CALIFA Team. Consejo Superior de Investigaciones Científicas. Estación Experimental de Zonas Aridas; España
description We study, for the first time in a statistically significant and well-defined sample, the relation between the outer-disk ionized-gas metallicity gradients and the presence of breaks in the surface brightness profiles of disk galaxies. Sloan Digital Sky Survey (SDSS) g′- and r′-band surface brightness, (g′ - r′) color, and ionized-gas oxygen abundance profiles for 324 galaxies within the Calar Alto Legacy Integral Field Area (CALIFA) survey are used for this purpose. We perform a detailed light-profile classification, finding that 84% of our disks show down- or up-bending profiles (Type II and Type III, respectively), while the remaining 16% are well fitted by one single exponential (Type I). The analysis of the color gradients at both sides of this break shows a U-shaped profile for most Type II galaxies with an average minimum (g′ - r′) color of ∼ 0.5mag and an ionized-gas metallicity flattening associated with it only in the case of low-mass galaxies. Comparatively, more massive systems show a rather uniform negative metallicity gradient. The correlation between metallicity flattening and stellar mass for these systems results in p-values as low as 0.01. Independent of the mechanism having shaped the outer light profiles of these galaxies, stellar migration or a previous episode of star formation in a shrinking star-forming disk, it is clear that the imprint in their ionized-gas metallicity was different for low- and high-mass Type II galaxies. In the case of Type III disks, a positive correlation between the change in color and abundance gradient is found (the null hypothesis is ruled out with a p-value of 0.02), with the outer disks of Type III galaxies with masses ≤1010 M′ showing a weak color reddening or even a bluing. This is interpreted as primarily due to a mass downsizing effect on the population of Type III galaxies that recently experienced an enhanced inside-out growth.
publishDate 2016
dc.date.none.fl_str_mv 2016-01-16
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/11336/78746
Marino, R. A.; Gil de Paz, A.; Sánchez, S. F.; Sanchez Blazquez, P.; Cardiel, N.; et al.; Outer-disk reddening and gas-phase metallicities: The CALIFA connection; EDP Sciences; Astronomy and Astrophysics; 585; 16-1-2016; 1-29
0004-6361
1432-0746
CONICET Digital
CONICET
url http://hdl.handle.net/11336/78746
identifier_str_mv Marino, R. A.; Gil de Paz, A.; Sánchez, S. F.; Sanchez Blazquez, P.; Cardiel, N.; et al.; Outer-disk reddening and gas-phase metallicities: The CALIFA connection; EDP Sciences; Astronomy and Astrophysics; 585; 16-1-2016; 1-29
0004-6361
1432-0746
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201526986
info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2016/01/aa26986-15/aa26986-15.html
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
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
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
_version_ 1844613733231362048
score 13.070432