SDSS-IV MaNGA : the role of the environment in AGN triggering

Detalhes bibliográficos
Autor(a) principal: Rembold, Sandro Barboza
Data de Publicação: 2024
Outros Autores: Riffel, Rogério, Riffel, Rogemar André, Storchi-Bergmann, Thaisa, Schimoia, Jáderson da Silva, Valk, Greique A., Lorenzoni, Vanessa, Ilha, Gabriele da Silva, Costa, Luiz N. da
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/278501
Resumo: The large- and small-scale environments around optically-selected AGN host galaxies and a controlsample of non-active galaxies in the MaNGA survey have been investigated in order to evaluate the importance of the environment in AGN triggering. Using the MaNGA integral field spectroscopy, we quantify non-circular motions of the ionized gas and detect an excess of radial gas motions in AGN hosts relative to control galaxies, not associated to AGN feedback and are most likely the result of tidal interactions, possibly associated with the triggering of the AGN. We find that the large-scale environments are similar for the AGN hosts and control galaxies in our sample and are biased towards lower large-scale densities and group virial masses, suggestive that the large-scale environment properties is only relevant to the AGN phenomenon in an indirect way, in the form, e.g. of the morphology-density relation. The small-scale environment, as measured by the frequency and luminosity of close neighbours, was also found to be similar for AGN and control galaxies. However, we find a correlation between the intensity of the noncircular gas motions in AGN hosts and the strength of the tidal field, while the control sample does not present such correlation. Also, AGN hosts with the most intense radial gas motions present larger tidal fields than their control galaxies. These findings indicate that at least a fraction of the AGN hosts in our sample have been triggered by tidal interactions with nearby galaxies.
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spelling Rembold, Sandro BarbozaRiffel, RogérioRiffel, Rogemar AndréStorchi-Bergmann, ThaisaSchimoia, Jáderson da SilvaValk, Greique A.Lorenzoni, VanessaIlha, Gabriele da SilvaCosta, Luiz N. da2024-09-06T06:39:09Z20240035-8711http://hdl.handle.net/10183/278501001198728The large- and small-scale environments around optically-selected AGN host galaxies and a controlsample of non-active galaxies in the MaNGA survey have been investigated in order to evaluate the importance of the environment in AGN triggering. Using the MaNGA integral field spectroscopy, we quantify non-circular motions of the ionized gas and detect an excess of radial gas motions in AGN hosts relative to control galaxies, not associated to AGN feedback and are most likely the result of tidal interactions, possibly associated with the triggering of the AGN. We find that the large-scale environments are similar for the AGN hosts and control galaxies in our sample and are biased towards lower large-scale densities and group virial masses, suggestive that the large-scale environment properties is only relevant to the AGN phenomenon in an indirect way, in the form, e.g. of the morphology-density relation. The small-scale environment, as measured by the frequency and luminosity of close neighbours, was also found to be similar for AGN and control galaxies. However, we find a correlation between the intensity of the noncircular gas motions in AGN hosts and the strength of the tidal field, while the control sample does not present such correlation. Also, AGN hosts with the most intense radial gas motions present larger tidal fields than their control galaxies. These findings indicate that at least a fraction of the AGN hosts in our sample have been triggered by tidal interactions with nearby galaxies.application/pdfengMonthly notices of the royal astronomical society. Oxford. Vol. 527, no. 3 (Jan. 2024), p. 6722–6731Galáxias ativasEvolucao galaticaGaláxiasGalaxies: activeGalaxies: evolutionGalaxies: groups: generalSDSS-IV MaNGA : the role of the environment in AGN triggeringEstrangeiroinfo: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:UFRGSTEXT001198728.pdf.txt001198728.pdf.txtExtracted Texttext/plain59521http://www.lume.ufrgs.br/bitstream/10183/278501/2/001198728.pdf.txt41c304d68e25c291e9f276cf6ba569bcMD52ORIGINAL001198728.pdfTexto completo (inglês)application/pdf1807099http://www.lume.ufrgs.br/bitstream/10183/278501/1/001198728.pdf16e7eaaccf059c2eb1d3a104ba352080MD5110183/2785012024-09-07 06:18:59.461334oai:www.lume.ufrgs.br:10183/278501Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2024-09-07T09:18:59Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv SDSS-IV MaNGA : the role of the environment in AGN triggering
title SDSS-IV MaNGA : the role of the environment in AGN triggering
spellingShingle SDSS-IV MaNGA : the role of the environment in AGN triggering
Rembold, Sandro Barboza
Galáxias ativas
Evolucao galatica
Galáxias
Galaxies: active
Galaxies: evolution
Galaxies: groups: general
title_short SDSS-IV MaNGA : the role of the environment in AGN triggering
title_full SDSS-IV MaNGA : the role of the environment in AGN triggering
title_fullStr SDSS-IV MaNGA : the role of the environment in AGN triggering
title_full_unstemmed SDSS-IV MaNGA : the role of the environment in AGN triggering
title_sort SDSS-IV MaNGA : the role of the environment in AGN triggering
author Rembold, Sandro Barboza
author_facet Rembold, Sandro Barboza
Riffel, Rogério
Riffel, Rogemar André
Storchi-Bergmann, Thaisa
Schimoia, Jáderson da Silva
Valk, Greique A.
Lorenzoni, Vanessa
Ilha, Gabriele da Silva
Costa, Luiz N. da
author_role author
author2 Riffel, Rogério
Riffel, Rogemar André
Storchi-Bergmann, Thaisa
Schimoia, Jáderson da Silva
Valk, Greique A.
Lorenzoni, Vanessa
Ilha, Gabriele da Silva
Costa, Luiz N. da
author2_role author
author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Rembold, Sandro Barboza
Riffel, Rogério
Riffel, Rogemar André
Storchi-Bergmann, Thaisa
Schimoia, Jáderson da Silva
Valk, Greique A.
Lorenzoni, Vanessa
Ilha, Gabriele da Silva
Costa, Luiz N. da
dc.subject.por.fl_str_mv Galáxias ativas
Evolucao galatica
Galáxias
topic Galáxias ativas
Evolucao galatica
Galáxias
Galaxies: active
Galaxies: evolution
Galaxies: groups: general
dc.subject.eng.fl_str_mv Galaxies: active
Galaxies: evolution
Galaxies: groups: general
description The large- and small-scale environments around optically-selected AGN host galaxies and a controlsample of non-active galaxies in the MaNGA survey have been investigated in order to evaluate the importance of the environment in AGN triggering. Using the MaNGA integral field spectroscopy, we quantify non-circular motions of the ionized gas and detect an excess of radial gas motions in AGN hosts relative to control galaxies, not associated to AGN feedback and are most likely the result of tidal interactions, possibly associated with the triggering of the AGN. We find that the large-scale environments are similar for the AGN hosts and control galaxies in our sample and are biased towards lower large-scale densities and group virial masses, suggestive that the large-scale environment properties is only relevant to the AGN phenomenon in an indirect way, in the form, e.g. of the morphology-density relation. The small-scale environment, as measured by the frequency and luminosity of close neighbours, was also found to be similar for AGN and control galaxies. However, we find a correlation between the intensity of the noncircular gas motions in AGN hosts and the strength of the tidal field, while the control sample does not present such correlation. Also, AGN hosts with the most intense radial gas motions present larger tidal fields than their control galaxies. These findings indicate that at least a fraction of the AGN hosts in our sample have been triggered by tidal interactions with nearby galaxies.
publishDate 2024
dc.date.accessioned.fl_str_mv 2024-09-06T06:39:09Z
dc.date.issued.fl_str_mv 2024
dc.type.driver.fl_str_mv Estrangeiro
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dc.language.iso.fl_str_mv eng
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dc.relation.ispartof.pt_BR.fl_str_mv Monthly notices of the royal astronomical society. Oxford. Vol. 527, no. 3 (Jan. 2024), p. 6722–6731
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