New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index

We derive a new relation between the metallicity of Seyfert 2 active galactic nuclei (AGNs) and the intensity of the narrow emission-lines ratio N2O2 = log([N II] λ6584/[O II] λ3727). The calibration of this relation was performed by determining the metallicity (Z) of a sample of 58 AGNs through a d...

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Detalles Bibliográficos
Autores principales: Castro, Cínthia S., Dors, Oli L., Cardaci, Mónica Viviana, Hägele, Guillermo Federico
Formato: Articulo
Lenguaje:Inglés
Publicado: 2017
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/123493
Aporte de:
id I19-R120-10915-123493
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Ciencias Exactas
Galaxies: abundances
Galaxies: evolution
Galaxies: formation
Galaxies: general
Galaxies: ISM
spellingShingle Ciencias Astronómicas
Ciencias Exactas
Galaxies: abundances
Galaxies: evolution
Galaxies: formation
Galaxies: general
Galaxies: ISM
Castro, Cínthia S.
Dors, Oli L.
Cardaci, Mónica Viviana
Hägele, Guillermo Federico
New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index
topic_facet Ciencias Astronómicas
Ciencias Exactas
Galaxies: abundances
Galaxies: evolution
Galaxies: formation
Galaxies: general
Galaxies: ISM
description We derive a new relation between the metallicity of Seyfert 2 active galactic nuclei (AGNs) and the intensity of the narrow emission-lines ratio N2O2 = log([N II] λ6584/[O II] λ3727). The calibration of this relation was performed by determining the metallicity (Z) of a sample of 58 AGNs through a diagram containing the observational data and the results of a grid of photoionization models obtained with the CLOUDY code. We find the new Z/Z⊙–N2O2 relation using the obtained metallicity values and the corresponding observational emission-line intensities for each object of the sample. Estimations derived through the use of this new calibration indicate that the narrow-line regions of Seyfert 2 galaxies exhibit a large range of metallicities (0.3 ≲ Z/Z⊙ ≲ 2.0), with a median value Z ≈ Z⊙. Regarding the possible existence of correlations between the luminosity L(Hβ), the electron density and the colour excess E(B − V) with the metallicity in this kind of objects, we do not find correlations between them.
format Articulo
Articulo
author Castro, Cínthia S.
Dors, Oli L.
Cardaci, Mónica Viviana
Hägele, Guillermo Federico
author_facet Castro, Cínthia S.
Dors, Oli L.
Cardaci, Mónica Viviana
Hägele, Guillermo Federico
author_sort Castro, Cínthia S.
title New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index
title_short New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index
title_full New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index
title_fullStr New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index
title_full_unstemmed New metallicity calibration for Seyfert 2 galaxies based on the N2O2 index
title_sort new metallicity calibration for seyfert 2 galaxies based on the n2o2 index
publishDate 2017
url http://sedici.unlp.edu.ar/handle/10915/123493
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AT dorsolil newmetallicitycalibrationforseyfert2galaxiesbasedonthen2o2index
AT cardacimonicaviviana newmetallicitycalibrationforseyfert2galaxiesbasedonthen2o2index
AT hageleguillermofederico newmetallicitycalibrationforseyfert2galaxiesbasedonthen2o2index
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