The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation
Autor(a) principal: | |
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Data de Publicação: | 2007 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/108962 |
Resumo: | We present the first detection of the near-infrared CN absorption band in the nuclear spectra of active galactic nuclei (AGNs). This feature is a recent star formation tracer, being particularly strong in carbon stars. The equivalent width of the CN line correlates with that of the CO at 2.3 μm as expected in stellar populations (SPs) with ages between ∼0.2 and ∼2 Gyr. The presence of the 1.1 μm CN band in the spectra of the sources is taken as unambiguous evidence of the presence of young/intermediate SPs close to the central source of the AGNs. Near-infrared bands can be powerful age indicators for star formation connected to AGNs, the understanding of which is crucial in the context of galaxy formation and AGN feedback. |
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Riffel, Rogemar AndréPastoriza, Miriani GriseldaRodriguez-Ardila, AlbertoMaraston, Claudia2015-01-15T02:15:05Z20070004-637Xhttp://hdl.handle.net/10183/108962000595774We present the first detection of the near-infrared CN absorption band in the nuclear spectra of active galactic nuclei (AGNs). This feature is a recent star formation tracer, being particularly strong in carbon stars. The equivalent width of the CN line correlates with that of the CO at 2.3 μm as expected in stellar populations (SPs) with ages between ∼0.2 and ∼2 Gyr. The presence of the 1.1 μm CN band in the spectra of the sources is taken as unambiguous evidence of the presence of young/intermediate SPs close to the central source of the AGNs. Near-infrared bands can be powerful age indicators for star formation connected to AGNs, the understanding of which is crucial in the context of galaxy formation and AGN feedback.application/pdfengThe Astrophysical journal. Chicago. Vol. 659, no. 2 pt. 2 (Apr. 2007), p. L103-L106Formacao de estrelasNucleo galaticoGaláxias ativasEspectros astronômicosCompostos de carbonoGalaxies: activeGalaxies: nucleiGalaxies: stellar contentThe first detection of near-infrared CN bands in active galactic nuclei : signature of star formationEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSORIGINAL000595774.pdf000595774.pdfTexto completo (inglês)application/pdf117299http://www.lume.ufrgs.br/bitstream/10183/108962/1/000595774.pdff53bad9182f28901b3ac6459ec5272e6MD51TEXT000595774.pdf.txt000595774.pdf.txtExtracted Texttext/plain20254http://www.lume.ufrgs.br/bitstream/10183/108962/2/000595774.pdf.txt51c6defdc9421de1c6e3032c1d78db34MD52THUMBNAIL000595774.pdf.jpg000595774.pdf.jpgGenerated Thumbnailimage/jpeg2043http://www.lume.ufrgs.br/bitstream/10183/108962/3/000595774.pdf.jpgf856a7e4ae8a879e5c712e7324076437MD5310183/1089622024-09-04 06:26:56.551878oai:www.lume.ufrgs.br:10183/108962Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2024-09-04T09:26:56Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation |
title |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation |
spellingShingle |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation Riffel, Rogemar André Formacao de estrelas Nucleo galatico Galáxias ativas Espectros astronômicos Compostos de carbono Galaxies: active Galaxies: nuclei Galaxies: stellar content |
title_short |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation |
title_full |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation |
title_fullStr |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation |
title_full_unstemmed |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation |
title_sort |
The first detection of near-infrared CN bands in active galactic nuclei : signature of star formation |
author |
Riffel, Rogemar André |
author_facet |
Riffel, Rogemar André Pastoriza, Miriani Griselda Rodriguez-Ardila, Alberto Maraston, Claudia |
author_role |
author |
author2 |
Pastoriza, Miriani Griselda Rodriguez-Ardila, Alberto Maraston, Claudia |
author2_role |
author author author |
dc.contributor.author.fl_str_mv |
Riffel, Rogemar André Pastoriza, Miriani Griselda Rodriguez-Ardila, Alberto Maraston, Claudia |
dc.subject.por.fl_str_mv |
Formacao de estrelas Nucleo galatico Galáxias ativas Espectros astronômicos Compostos de carbono |
topic |
Formacao de estrelas Nucleo galatico Galáxias ativas Espectros astronômicos Compostos de carbono Galaxies: active Galaxies: nuclei Galaxies: stellar content |
dc.subject.eng.fl_str_mv |
Galaxies: active Galaxies: nuclei Galaxies: stellar content |
description |
We present the first detection of the near-infrared CN absorption band in the nuclear spectra of active galactic nuclei (AGNs). This feature is a recent star formation tracer, being particularly strong in carbon stars. The equivalent width of the CN line correlates with that of the CO at 2.3 μm as expected in stellar populations (SPs) with ages between ∼0.2 and ∼2 Gyr. The presence of the 1.1 μm CN band in the spectra of the sources is taken as unambiguous evidence of the presence of young/intermediate SPs close to the central source of the AGNs. Near-infrared bands can be powerful age indicators for star formation connected to AGNs, the understanding of which is crucial in the context of galaxy formation and AGN feedback. |
publishDate |
2007 |
dc.date.issued.fl_str_mv |
2007 |
dc.date.accessioned.fl_str_mv |
2015-01-15T02:15:05Z |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/108962 |
dc.identifier.issn.pt_BR.fl_str_mv |
0004-637X |
dc.identifier.nrb.pt_BR.fl_str_mv |
000595774 |
identifier_str_mv |
0004-637X 000595774 |
url |
http://hdl.handle.net/10183/108962 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
The Astrophysical journal. Chicago. Vol. 659, no. 2 pt. 2 (Apr. 2007), p. L103-L106 |
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info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
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application/pdf |
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