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dc.rights.license© G. Venturi et al. 2021es
dc.contributor.authorVenturi, G.-
dc.contributor.authorCresci, G.-
dc.contributor.authorMarconi, A.-
dc.contributor.authorMingozzi, M.-
dc.contributor.authorNardini, E.-
dc.contributor.authorCarniani, S.-
dc.contributor.authorMannucci, F.-
dc.contributor.authorMarasco, A.-
dc.contributor.authorMaiolino, R.-
dc.contributor.authorPerna, M.-
dc.contributor.authorTreister, E.-
dc.contributor.authorBland Hawthorn, J.-
dc.contributor.authorGallimore, J.-
dc.date.accessioned2022-02-14T11:19:49Z-
dc.date.available2022-02-14T11:19:49Z-
dc.date.issued2021-04-07-
dc.identifier.citationAstronomy and Astrophysics 648: A17(2021)es
dc.identifier.issn0004-6361-
dc.identifier.otherhttps://www.aanda.org/articles/aa/full_html/2021/04/aa39869-20/aa39869-20.html-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/543-
dc.descriptionBased on observations made with ESO Telescopes at the La Silla Paranal Observatory under program IDs 094.B-0321, 60.A-9339, 095.B-0532.es
dc.description.abstractContext. Outflows accelerated by active galactic nuclei (AGN) are commonly observed in the form of coherent, mildly collimated high-velocity gas directed along the AGN ionisation cones and kinetically powerful (≳1044 − 45 erg s−1) jets. Recent works found that outflows can also be accelerated by low-power (≲1044 erg s−1) jets, and the most recent cosmological simulations indicate that these are the dominant source of feedback on sub-kiloparsec scales, but little is known about their effect on the galaxy host. Aims. We study the relation between radio jets and the distribution and kinematics of the ionised gas in IC 5063, NGC 5643, NGC 1068, and NGC 1386 as part of our survey of nearby Seyfert galaxies called Measuring Active Galactic Nuclei Under MUSE Microscope (MAGNUM). All these objects host a small-scale (≲1 kpc) low-power (≲1044 erg s−1) radio jet that has small inclinations (≲45°) with respect to the galaxy disc. Methods. We employed seeing-limited optical integral field spectroscopic observations from the Multi Unit Spectroscopic Explorer (MUSE) at the Very Large Telescope to obtain flux, kinematic, and excitation maps of the extended ionised gas. We compared these maps with archival radio images and in one case, with Chandra X-ray observations. Results. We detect a strong (up to ≳800–1000 km s−1) and extended (≳1 kpc) emission-line velocity spread perpendicular to the direction of the AGN ionisation cones and jets in all four targets. The gas excitation in this region of line-width enhancement is entirely compatible with shock ionisation. These broad and symmetric line profiles are not associated with a single coherent velocity of the gas. A ‘classical’ outflow component with net blueshifted and redshifted motions is also present, but is directed along the ionisation cones and jets. Conclusions. We interpret the observed phenomenon as due to the action of the jets perturbing the gas in the galaxy disc. These intense and extended velocity spreads perpendicular to AGN jets and cones are indeed currently only observed in galaxies hosting a low-power jet whose inclination is sufficiently low with respect to the galaxy disc to impact on and strongly affect its material. In line with cosmological simulations, our results demonstrate that low-power jets are indeed capable of affecting the host galaxy.es
dc.description.sponsorshipWe acknowledge support from ANID programs FONDECYT Postdoctorado 3200802 (G. V.), Basal-CATA AFB-170002 (G. V. and E. T.), FONDECYT Regular 1190818 (E. T.) and Anillo ACT172033 (E. T.). G. C. and Al. M. acknowledge support from PRIN MIUR project Black Hole winds and the Baryon Life Cycle of Galaxies: the stone-guest at the galaxy evolution supper, contract #2017PH3WAT. M. P. is supported by the Programa Atraccion de Talento de la Comunidad de Madrid via grant 2018-T2/TIC-11715. R. M. acknowledges ERC Advanced Grant 695671 QUENCH and support by the Science and Technology Facilities Council (STFC). This research has made use of the services of the ESO Science Archive Facility. The scientific results reported in this article are based in part on data obtained from the Chandra Data Archive (ObsID: 344). This research has made use of software provided by the Chandra X-ray Center (CXC) in the application package CIAO. This research has made use of NASA's Astrophysics Data System Bibliographic Services. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is funded by the National Aeronautics and Space Administration and operated by the California Institute of Technology. We acknowledge the usage of the HyperLeda database (http://leda.univ-lyon1.fr; Makarov et al. 2014). This research has made use of Aladin sky atlas developed at CDS, Strasbourg Observatory, France (Bonnarel et al. 2000). This research made use of the Python packages SciPy (Virtanen et al. 2020), NumPy (Harris et al. 2020), IPython (Perez & Granger 2007) and Matplotlib (Hunter 2007). This research made use of Astropy (http://www.astropy.org), a community-developed core Python package for Astronomy (Astropy Collaboration 2013, 2018). The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. The Australia Telescope Compact Array is part of the Australia Telescope National Facility which is funded by the Australian Government for operation as a National Facility managed by CSIRO. We thank Ra ffaella Morganti for the fruitful discussion on this work and for having provided the ATCA radio data of IC 5063. We thank Dipanjan Mukherjee for the useful insights regarding jet-ISM simulations. We thank Tanya Urrutia for her contribution to the earliest work on the MAGNUM project.es
dc.language.isoenges
dc.publisherEDP Scienceses
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/-
dc.subjectGalaxies: seyfertes
dc.subjectGalaxies: jetses
dc.subjectGalaxies: activees
dc.subjectGalaxies: ISMes
dc.subjectTechniques: imaging spectroscopyes
dc.titleMAGNUM survey: Compact jets causing large turmoil in galaxies Enhanced line widths perpendicular to radio jets as tracers of jet-ISM interactiones
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidVenturi, G. [0000-0001-8349-3055]-
dc.contributor.orcidCresci, G. [0000-0002-5281-1417]-
dc.contributor.orcidMarconi, A. [0000-0002-9889-4238]-
dc.contributor.orcidMingozzi, M. [0000-0003-2589-762X]-
dc.contributor.orcidNardini, E. [0000-0001-9226-8992]-
dc.contributor.orcidCarniani, S. [0000-0002-6719-380X]-
dc.contributor.orcidMannucci, F. [0000-0002-4803-2381]-
dc.contributor.orcidMarasco, A. [0000-0002-5655-6054]-
dc.contributor.orcidPerna, M. [0000-0002-0362-5941]-
dc.contributor.orcidTreister, E. [0000-0001-7568-6412]-
dc.contributor.orcidGallimore, J. [0000-0002-6972-2760]-
dc.identifier.doi10.1051/0004-6361/202039869-
dc.identifier.e-issn1432-0746-
dc.contributor.funderFondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)-
dc.contributor.funderEuropean Research Council (ERC)-
dc.contributor.funderScience and Technology Facilities Council (STFC)-
dc.contributor.funderComunidad de Madrid-
dc.description.peerreviewedPeerreviewes
dc.identifier.funderhttp://dx.doi.org/10.13039/501100002850-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000781-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000271-
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/695671-
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