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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/78746
Ver los metadatos del registro completo
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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 Técnicas2025-10-15T14:53:30Zoai: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:34982025-10-15 14:53:31.082CONICET 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 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://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 |
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eng |
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eng |
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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 |
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openAccess |
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EDP Sciences |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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