X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies
- Autores
- Dors Junior, Oli L.; Riffel, Rogemar A.; Cardaci, Mónica Viviana; Hägele, Guillermo Federico; Krabbe, Angela Cristina; Pérez Montero, Enrique; Rodrigues, Irapuan
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We investigate the excitation mechanisms of near-infrared [Fe II] and H2 emission lines observed in active galactic nuclei (AGNs). We built a photoionization model grid considering a two-component continuum: one component accounts for the 'big bump' component peaking at 1Ryd and another represents the X-ray source that dominates the continuum emission at high energies. Photoionization models considering as ionizing source a spectral energy distribution obtained from photometric data of Seyert 2 Mrk1066 taken from the literature were considered. Results of these models were compared with a large sample of observational long-slit and Integral field Unit (IFU) spectroscopy data of the nuclear region for a sample of active objects. We found that the correlation between the observational [Fe II]λ 1.2570μm/Paβ and H2λ2.1218μm/Brγ is well reproduced by our models, as are the relationships that involve the H2 emission-line ratios observed in the spectroscopic data. We conclude that heating by X-rays produced by active nuclei can be considered a common and very important mechanism of excitation of [Fe II] and H2.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Galaxies: ISM
Galaxies: Seyfert
Infrared: galaxies - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/83917
Ver los metadatos del registro completo
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X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxiesDors Junior, Oli L.Riffel, Rogemar A.Cardaci, Mónica VivianaHägele, Guillermo FedericoKrabbe, Angela CristinaPérez Montero, EnriqueRodrigues, IrapuanCiencias AstronómicasGalaxies: ISMGalaxies: SeyfertInfrared: galaxiesWe investigate the excitation mechanisms of near-infrared [Fe II] and H<SUB>2</SUB> emission lines observed in active galactic nuclei (AGNs). We built a photoionization model grid considering a two-component continuum: one component accounts for the 'big bump' component peaking at 1Ryd and another represents the X-ray source that dominates the continuum emission at high energies. Photoionization models considering as ionizing source a spectral energy distribution obtained from photometric data of Seyert 2 Mrk1066 taken from the literature were considered. Results of these models were compared with a large sample of observational long-slit and Integral field Unit (IFU) spectroscopy data of the nuclear region for a sample of active objects. We found that the correlation between the observational [Fe II]λ 1.2570μm/Paβ and H<SUB>2</SUB>λ2.1218μm/Brγ is well reproduced by our models, as are the relationships that involve the H<SUB>2</SUB> emission-line ratios observed in the spectroscopic data. We conclude that heating by X-rays produced by active nuclei can be considered a common and very important mechanism of excitation of [Fe II] and H<SUB>2</SUB>.Facultad de Ciencias Astronómicas y Geofísicas2012info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf252-260http://sedici.unlp.edu.ar/handle/10915/83917enginfo:eu-repo/semantics/altIdentifier/issn/0035-8711info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2012.20600.xinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:16:05Zoai:sedici.unlp.edu.ar:10915/83917Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:05.407SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies |
title |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies |
spellingShingle |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies Dors Junior, Oli L. Ciencias Astronómicas Galaxies: ISM Galaxies: Seyfert Infrared: galaxies |
title_short |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies |
title_full |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies |
title_fullStr |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies |
title_full_unstemmed |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies |
title_sort |
X-rays as the dominant excitation mechanism of [Fe II] and H2 emission lines in active galaxies |
dc.creator.none.fl_str_mv |
Dors Junior, Oli L. Riffel, Rogemar A. Cardaci, Mónica Viviana Hägele, Guillermo Federico Krabbe, Angela Cristina Pérez Montero, Enrique Rodrigues, Irapuan |
author |
Dors Junior, Oli L. |
author_facet |
Dors Junior, Oli L. Riffel, Rogemar A. Cardaci, Mónica Viviana Hägele, Guillermo Federico Krabbe, Angela Cristina Pérez Montero, Enrique Rodrigues, Irapuan |
author_role |
author |
author2 |
Riffel, Rogemar A. Cardaci, Mónica Viviana Hägele, Guillermo Federico Krabbe, Angela Cristina Pérez Montero, Enrique Rodrigues, Irapuan |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Galaxies: ISM Galaxies: Seyfert Infrared: galaxies |
topic |
Ciencias Astronómicas Galaxies: ISM Galaxies: Seyfert Infrared: galaxies |
dc.description.none.fl_txt_mv |
We investigate the excitation mechanisms of near-infrared [Fe II] and H<SUB>2</SUB> emission lines observed in active galactic nuclei (AGNs). We built a photoionization model grid considering a two-component continuum: one component accounts for the 'big bump' component peaking at 1Ryd and another represents the X-ray source that dominates the continuum emission at high energies. Photoionization models considering as ionizing source a spectral energy distribution obtained from photometric data of Seyert 2 Mrk1066 taken from the literature were considered. Results of these models were compared with a large sample of observational long-slit and Integral field Unit (IFU) spectroscopy data of the nuclear region for a sample of active objects. We found that the correlation between the observational [Fe II]λ 1.2570μm/Paβ and H<SUB>2</SUB>λ2.1218μm/Brγ is well reproduced by our models, as are the relationships that involve the H<SUB>2</SUB> emission-line ratios observed in the spectroscopic data. We conclude that heating by X-rays produced by active nuclei can be considered a common and very important mechanism of excitation of [Fe II] and H<SUB>2</SUB>. Facultad de Ciencias Astronómicas y Geofísicas |
description |
We investigate the excitation mechanisms of near-infrared [Fe II] and H<SUB>2</SUB> emission lines observed in active galactic nuclei (AGNs). We built a photoionization model grid considering a two-component continuum: one component accounts for the 'big bump' component peaking at 1Ryd and another represents the X-ray source that dominates the continuum emission at high energies. Photoionization models considering as ionizing source a spectral energy distribution obtained from photometric data of Seyert 2 Mrk1066 taken from the literature were considered. Results of these models were compared with a large sample of observational long-slit and Integral field Unit (IFU) spectroscopy data of the nuclear region for a sample of active objects. We found that the correlation between the observational [Fe II]λ 1.2570μm/Paβ and H<SUB>2</SUB>λ2.1218μm/Brγ is well reproduced by our models, as are the relationships that involve the H<SUB>2</SUB> emission-line ratios observed in the spectroscopic data. We conclude that heating by X-rays produced by active nuclei can be considered a common and very important mechanism of excitation of [Fe II] and H<SUB>2</SUB>. |
publishDate |
2012 |
dc.date.none.fl_str_mv |
2012 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/83917 |
url |
http://sedici.unlp.edu.ar/handle/10915/83917 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0035-8711 info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2012.20600.x |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
eu_rights_str_mv |
openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
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