Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates

Autores
Dors, Oli L.; Valerdi Manuel, Carlos Julián; Riffel, R. A.; Riffel, R.; Cardaci, Monica Viviana; Hägele, Guillermo Federico; Armah, Mark; Revalski, M.; Flury, S. R.; Freitas Lemes, P.; Amôres, E. B.; Krabbe, A. C.; Binette, L.; Feltre, A.; Storchi Bergmann, T.
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
For the first time, the sulphur abundance relative to hydrogen (S/H) in the Narrow Line Regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the electron temperature. Narrow emission line intensities from the SDSS considered. Our direct estimates indicate that Sy 2s have similar temperatures in the gas region where most of the S ions are located in comparison with that of star-forming regions (SFs). However, Sy 2s present higher temperature values (∼ 10 000 K) in the region where most of the S2+ ions are located relative to that of SFs. We derive the total sulphur abundance in the range of 6.2 ∼< 12 + log(S/H) ∼< 7.5, corresponding to 0.1 - 1.8 times the solar value. These sulphur abundance values are lower by ∼ 0.4 dex than those derived in SFs with similar metallicity, indicating a distinct chemical enrichment of the ISM for these object classes. The S/O values for our Sy 2 sample present an abrupt (∼ 0.5 dex) decrease with increasing O/H for the high metallicity regime [12 + log(O/H) ∼> 8.7)], what is not seen for the SFs. However, when our Sy 2 estimates are combined with those from a large sample of star-forming regions, we did not find any dependence between S/O and O/H.
Fil: Dors, Oli L.. Universidade Do Vale Do Paraíba; Brasil
Fil: Valerdi Manuel, Carlos Julián. Instituto Nacional de Astrofísica Óptica y Electrónica; México
Fil: Riffel, R. A.. Universidade Federal de Santa Maria; Brasil
Fil: Riffel, R.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Cardaci, Monica Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Armah, Mark. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Revalski, M.. Space Telescope Science Institute; Estados Unidos
Fil: Flury, S. R.. University of Massachussets; Estados Unidos
Fil: Freitas Lemes, P.. Universidade Do Vale Do Paraíba; Brasil
Fil: Amôres, E. B.. Universidade Estadual de Feira de Santana; Brasil
Fil: Krabbe, A. C.. Universidade Do Vale Do Paraíba; Brasil
Fil: Binette, L.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Fil: Feltre, A.. Osservatorio Di Astrofisica E Scienza Dello Spazio; Italia
Fil: Storchi Bergmann, T.. Universidade Federal do Rio Grande do Sul; Brasil
Materia
galaxies: Seyfert
galaxies: active
galaxies: 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:11336/232885
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/232885
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimatesDors, Oli L.Valerdi Manuel, Carlos JuliánRiffel, R. A.Riffel, R.Cardaci, Monica VivianaHägele, Guillermo FedericoArmah, MarkRevalski, M.Flury, S. R.Freitas Lemes, P.Amôres, E. B.Krabbe, A. C.Binette, L.Feltre, A.Storchi Bergmann, T.galaxies: Seyfertgalaxies: activegalaxies: abundanceshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1For the first time, the sulphur abundance relative to hydrogen (S/H) in the Narrow Line Regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the electron temperature. Narrow emission line intensities from the SDSS considered. Our direct estimates indicate that Sy 2s have similar temperatures in the gas region where most of the S ions are located in comparison with that of star-forming regions (SFs). However, Sy 2s present higher temperature values (∼ 10 000 K) in the region where most of the S2+ ions are located relative to that of SFs. We derive the total sulphur abundance in the range of 6.2 ∼< 12 + log(S/H) ∼< 7.5, corresponding to 0.1 - 1.8 times the solar value. These sulphur abundance values are lower by ∼ 0.4 dex than those derived in SFs with similar metallicity, indicating a distinct chemical enrichment of the ISM for these object classes. The S/O values for our Sy 2 sample present an abrupt (∼ 0.5 dex) decrease with increasing O/H for the high metallicity regime [12 + log(O/H) ∼> 8.7)], what is not seen for the SFs. However, when our Sy 2 estimates are combined with those from a large sample of star-forming regions, we did not find any dependence between S/O and O/H.Fil: Dors, Oli L.. Universidade Do Vale Do Paraíba; BrasilFil: Valerdi Manuel, Carlos Julián. Instituto Nacional de Astrofísica Óptica y Electrónica; MéxicoFil: Riffel, R. A.. Universidade Federal de Santa Maria; BrasilFil: Riffel, R.. Universidade Federal do Rio Grande do Sul; BrasilFil: Cardaci, Monica Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Armah, Mark. Universidade Federal do Rio Grande do Sul; BrasilFil: Revalski, M.. Space Telescope Science Institute; Estados UnidosFil: Flury, S. R.. University of Massachussets; Estados UnidosFil: Freitas Lemes, P.. Universidade Do Vale Do Paraíba; BrasilFil: Amôres, E. B.. Universidade Estadual de Feira de Santana; BrasilFil: Krabbe, A. C.. Universidade Do Vale Do Paraíba; BrasilFil: Binette, L.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; MéxicoFil: Feltre, A.. Osservatorio Di Astrofisica E Scienza Dello Spazio; ItaliaFil: Storchi Bergmann, T.. Universidade Federal do Rio Grande do Sul; BrasilWiley Blackwell Publishing, Inc2023-05info: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/11336/232885Dors, Oli L.; Valerdi Manuel, Carlos Julián; Riffel, R. A.; Riffel, R.; Cardaci, Monica Viviana; et al.; Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 521; 2; 5-2023; 1969-19870035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/521/2/1969/7068106info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad635info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:45:30Zoai:ri.conicet.gov.ar:11336/232885instacron: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:34982025-09-03 09:45:30.466CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
title Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
spellingShingle Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
Dors, Oli L.
galaxies: Seyfert
galaxies: active
galaxies: abundances
title_short Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
title_full Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
title_fullStr Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
title_full_unstemmed Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
title_sort Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates
dc.creator.none.fl_str_mv Dors, Oli L.
Valerdi Manuel, Carlos Julián
Riffel, R. A.
Riffel, R.
Cardaci, Monica Viviana
Hägele, Guillermo Federico
Armah, Mark
Revalski, M.
Flury, S. R.
Freitas Lemes, P.
Amôres, E. B.
Krabbe, A. C.
Binette, L.
Feltre, A.
Storchi Bergmann, T.
author Dors, Oli L.
author_facet Dors, Oli L.
Valerdi Manuel, Carlos Julián
Riffel, R. A.
Riffel, R.
Cardaci, Monica Viviana
Hägele, Guillermo Federico
Armah, Mark
Revalski, M.
Flury, S. R.
Freitas Lemes, P.
Amôres, E. B.
Krabbe, A. C.
Binette, L.
Feltre, A.
Storchi Bergmann, T.
author_role author
author2 Valerdi Manuel, Carlos Julián
Riffel, R. A.
Riffel, R.
Cardaci, Monica Viviana
Hägele, Guillermo Federico
Armah, Mark
Revalski, M.
Flury, S. R.
Freitas Lemes, P.
Amôres, E. B.
Krabbe, A. C.
Binette, L.
Feltre, A.
Storchi Bergmann, T.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv galaxies: Seyfert
galaxies: active
galaxies: abundances
topic galaxies: Seyfert
galaxies: active
galaxies: 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 For the first time, the sulphur abundance relative to hydrogen (S/H) in the Narrow Line Regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the electron temperature. Narrow emission line intensities from the SDSS considered. Our direct estimates indicate that Sy 2s have similar temperatures in the gas region where most of the S ions are located in comparison with that of star-forming regions (SFs). However, Sy 2s present higher temperature values (∼ 10 000 K) in the region where most of the S2+ ions are located relative to that of SFs. We derive the total sulphur abundance in the range of 6.2 ∼< 12 + log(S/H) ∼< 7.5, corresponding to 0.1 - 1.8 times the solar value. These sulphur abundance values are lower by ∼ 0.4 dex than those derived in SFs with similar metallicity, indicating a distinct chemical enrichment of the ISM for these object classes. The S/O values for our Sy 2 sample present an abrupt (∼ 0.5 dex) decrease with increasing O/H for the high metallicity regime [12 + log(O/H) ∼> 8.7)], what is not seen for the SFs. However, when our Sy 2 estimates are combined with those from a large sample of star-forming regions, we did not find any dependence between S/O and O/H.
Fil: Dors, Oli L.. Universidade Do Vale Do Paraíba; Brasil
Fil: Valerdi Manuel, Carlos Julián. Instituto Nacional de Astrofísica Óptica y Electrónica; México
Fil: Riffel, R. A.. Universidade Federal de Santa Maria; Brasil
Fil: Riffel, R.. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Cardaci, Monica Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Hägele, Guillermo Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Armah, Mark. Universidade Federal do Rio Grande do Sul; Brasil
Fil: Revalski, M.. Space Telescope Science Institute; Estados Unidos
Fil: Flury, S. R.. University of Massachussets; Estados Unidos
Fil: Freitas Lemes, P.. Universidade Do Vale Do Paraíba; Brasil
Fil: Amôres, E. B.. Universidade Estadual de Feira de Santana; Brasil
Fil: Krabbe, A. C.. Universidade Do Vale Do Paraíba; Brasil
Fil: Binette, L.. Universidad Nacional Autonoma de Mexico. Instituto de Astronomia; México
Fil: Feltre, A.. Osservatorio Di Astrofisica E Scienza Dello Spazio; Italia
Fil: Storchi Bergmann, T.. Universidade Federal do Rio Grande do Sul; Brasil
description For the first time, the sulphur abundance relative to hydrogen (S/H) in the Narrow Line Regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the electron temperature. Narrow emission line intensities from the SDSS considered. Our direct estimates indicate that Sy 2s have similar temperatures in the gas region where most of the S ions are located in comparison with that of star-forming regions (SFs). However, Sy 2s present higher temperature values (∼ 10 000 K) in the region where most of the S2+ ions are located relative to that of SFs. We derive the total sulphur abundance in the range of 6.2 ∼< 12 + log(S/H) ∼< 7.5, corresponding to 0.1 - 1.8 times the solar value. These sulphur abundance values are lower by ∼ 0.4 dex than those derived in SFs with similar metallicity, indicating a distinct chemical enrichment of the ISM for these object classes. The S/O values for our Sy 2 sample present an abrupt (∼ 0.5 dex) decrease with increasing O/H for the high metallicity regime [12 + log(O/H) ∼> 8.7)], what is not seen for the SFs. However, when our Sy 2 estimates are combined with those from a large sample of star-forming regions, we did not find any dependence between S/O and O/H.
publishDate 2023
dc.date.none.fl_str_mv 2023-05
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/11336/232885
Dors, Oli L.; Valerdi Manuel, Carlos Julián; Riffel, R. A.; Riffel, R.; Cardaci, Monica Viviana; et al.; Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 521; 2; 5-2023; 1969-1987
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/232885
identifier_str_mv Dors, Oli L.; Valerdi Manuel, Carlos Julián; Riffel, R. A.; Riffel, R.; Cardaci, Monica Viviana; et al.; Chemical abundances in Seyfert galaxies – X. Sulphur abundance estimates; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 521; 2; 5-2023; 1969-1987
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/url/https://academic.oup.com/mnras/article/521/2/1969/7068106
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stad635
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 Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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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score 13.13397

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