Galaxy-wide radio-induced feedback in a radio-quiet quasar.

We report the discovery of a radio-quiet type 2 quasar (SDSS J165315.06+234943.0 nicknamed the 'Beetle' at z=0.103) with unambiguous evidence for active galactic nucleus (AGN) radio-induced feedback acting across a total extension of ~46 kpc and up to ~26 kpc from the AGN. To the best of o...

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Autores: Villar-Martín, M., Emonts, Bjorn H. C., Cabrera-Lavers, Antonio, Tadhunter, Clive, Mukherjee, D., Humphrey, Andrew, Rodríguez Zaurín, Javier, Ramos Almeida, C., Pérez-Torres, Miguel A., Bessiere, P. S.
Tipo de documento: artigo
Estado:Versão publicada
Data de publicação:2017
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositório:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/370462
Acesso em linha:http://hdl.handle.net/10261/370462
Access Level:Acceso aberto
Palavra-chave:Galaxies: active
Galaxies: evolution
Guasars: individual: SDSS J1653+23
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dc.title.none.fl_str_mv Galaxy-wide radio-induced feedback in a radio-quiet quasar.
title Galaxy-wide radio-induced feedback in a radio-quiet quasar.
spellingShingle Galaxy-wide radio-induced feedback in a radio-quiet quasar.
Villar-Martín, M.
Galaxies: active
Galaxies: evolution
Guasars: individual: SDSS J1653+23
title_short Galaxy-wide radio-induced feedback in a radio-quiet quasar.
title_full Galaxy-wide radio-induced feedback in a radio-quiet quasar.
title_fullStr Galaxy-wide radio-induced feedback in a radio-quiet quasar.
title_full_unstemmed Galaxy-wide radio-induced feedback in a radio-quiet quasar.
title_sort Galaxy-wide radio-induced feedback in a radio-quiet quasar.
dc.creator.none.fl_str_mv Villar-Martín, M.
Emonts, Bjorn H. C.
Cabrera-Lavers, Antonio
Tadhunter, Clive
Mukherjee, D.
Humphrey, Andrew
Rodríguez Zaurín, Javier
Ramos Almeida, C.
Pérez-Torres, Miguel A.
Bessiere, P. S.
author Villar-Martín, M.
author_facet Villar-Martín, M.
Emonts, Bjorn H. C.
Cabrera-Lavers, Antonio
Tadhunter, Clive
Mukherjee, D.
Humphrey, Andrew
Rodríguez Zaurín, Javier
Ramos Almeida, C.
Pérez-Torres, Miguel A.
Bessiere, P. S.
author_role author
author2 Emonts, Bjorn H. C.
Cabrera-Lavers, Antonio
Tadhunter, Clive
Mukherjee, D.
Humphrey, Andrew
Rodríguez Zaurín, Javier
Ramos Almeida, C.
Pérez-Torres, Miguel A.
Bessiere, P. S.
author2_role author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Ministerio de Economía y Competitividad (España)
Fundação para a Ciência e a Tecnologia (Portugal)
European Commission
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Galaxies: active
Galaxies: evolution
Guasars: individual: SDSS J1653+23
topic Galaxies: active
Galaxies: evolution
Guasars: individual: SDSS J1653+23
description We report the discovery of a radio-quiet type 2 quasar (SDSS J165315.06+234943.0 nicknamed the 'Beetle' at z=0.103) with unambiguous evidence for active galactic nucleus (AGN) radio-induced feedback acting across a total extension of ~46 kpc and up to ~26 kpc from the AGN. To the best of our knowledge, this is the first radio-quiet system where radio-induced feedback has been securely identified at »several kpc from the AGN. The morphological, ionization and kinematic properties of the extended ionized gas are correlated with the radio structures. We find along the radio axis (a) enhancement of the optical line emission at the location of the radio hotspots (b) turbulent gas kinematics (FWHM ~ 380-470 km s-1) across the entire spatial range circumscribed by them (c) ionization minima for the turbulent gas at the location of the hot spots, (d) high temperature Te ¿ 1.9 × 104 K at the NE hotspot. Turbulent gas is also found far from the radio axis, ~25 kpc in the perpendicular direction.We propose a scenario in which the radio structures have perforated the interstellar medium of the galaxy and escaped into the circumgalactic medium. While advancing, they have interacted with in situ gas modifying its properties. Our results show that jets of modest power can be the dominant feedback mechanism acting across huge volumes in radio-quiet systems, including highly accreting luminous AGNs, where radiative mode feedback may be expected. © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society
publishDate 2017
dc.date.none.fl_str_mv 2017
2024
2024
2024
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dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/370462
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dc.language.none.fl_str_mv Inglés
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dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
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dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
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spelling Galaxy-wide radio-induced feedback in a radio-quiet quasar.Villar-Martín, M.Emonts, Bjorn H. C.Cabrera-Lavers, AntonioTadhunter, CliveMukherjee, D.Humphrey, AndrewRodríguez Zaurín, JavierRamos Almeida, C.Pérez-Torres, Miguel A.Bessiere, P. S.Galaxies: activeGalaxies: evolutionGuasars: individual: SDSS J1653+23We report the discovery of a radio-quiet type 2 quasar (SDSS J165315.06+234943.0 nicknamed the 'Beetle' at z=0.103) with unambiguous evidence for active galactic nucleus (AGN) radio-induced feedback acting across a total extension of ~46 kpc and up to ~26 kpc from the AGN. To the best of our knowledge, this is the first radio-quiet system where radio-induced feedback has been securely identified at »several kpc from the AGN. The morphological, ionization and kinematic properties of the extended ionized gas are correlated with the radio structures. We find along the radio axis (a) enhancement of the optical line emission at the location of the radio hotspots (b) turbulent gas kinematics (FWHM ~ 380-470 km s-1) across the entire spatial range circumscribed by them (c) ionization minima for the turbulent gas at the location of the hot spots, (d) high temperature Te ¿ 1.9 × 104 K at the NE hotspot. Turbulent gas is also found far from the radio axis, ~25 kpc in the perpendicular direction.We propose a scenario in which the radio structures have perforated the interstellar medium of the galaxy and escaped into the circumgalactic medium. While advancing, they have interacted with in situ gas modifying its properties. Our results show that jets of modest power can be the dominant feedback mechanism acting across huge volumes in radio-quiet systems, including highly accreting luminous AGNs, where radiative mode feedback may be expected. © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. © 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical SocietyThis work is based on observations carried out at the Observatorio Roque de los Muchachos (La Palma, Spain) with OSIRIS on GTC (programmes GTC37/14A, GTC1/15A and GTC01-16ADDT) and the Very Large Array (programmes VLA/15A-237 and VLA/16A- 088). Partly based on observations made with the GTC telescope, under Director’s Discretionary Time. We thank the GTC staff for their support with the optical imaging and spectroscopic observa- tions and the VLA staff for executing the radio observations. Thanks to Gustaaf van Moorsel for his valuable advice about the radio ob- servations. MVM, AC and BE acknowledge support from the Spanish Ministerio de Econom´ıa y Competitividad through the grants AYA2015-64346-C2-2-P and AYA2012-32295. AH acknowledges Fundac¸ ˜ao para a Ciˆencia e a Tecnologia (FCT) support through UID/FIS/04434/2013, and through project FCOMP-01-0124- FEDER-029170 (Reference FCT PTDC/FIS-AST/3214/2012) funded by FCT-MEC (PIDDAC) and FEDER (COMPETE), in ad- dition to FP7 project PIRSES-GA-2013-612701. AH also acknowl- edges a Marie Curie Fellowship co-funded by the FP7 and the FCT (DFRH/WIIA/57/2011) and FP7 / FCT Complementary Sup- port grant SFRH/BI/52155/2013. BE acknowledges support from the European Union 7th Framework Programme (FP7-PEOPLE- 2013-IEF) under grant 624351. CRA acknowledges the Ram´on y Cajal Programme of the Spanish Ministry of Economy and Com- petitiveness through project RYC-2014-15779 and the Spanish Plan Nacional de Astronom´ıa y Astrofis´ıca under grant AYA2016-76682- C3-2-P. This research has used the following: (1) The VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in Ochsenbein et al. (2000). (2) The NASA/IPAC circumgalactic Database (NED) that is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administra- tion. (3) Data from Sloan Digital Sky Survey. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/.Oxford University PressMinisterio de Economía y Competitividad (España)Fundação para a Ciência e a Tecnologia (Portugal)European CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2024202420172024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/370462reponame:DIGITAL.CSIC. 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