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dc.rights.license© ESO 2021-
dc.contributor.authorTozzi, P.-
dc.contributor.authorCresci, G.-
dc.contributor.authorMarasco, A.-
dc.contributor.authorNardini, E.-
dc.contributor.authorMarconi, A.-
dc.contributor.authorMannucci, F.-
dc.contributor.authorChartas, G.-
dc.contributor.authorRizzo, F.-
dc.contributor.authorAmiri, A.-
dc.contributor.authorBrusa, M.-
dc.contributor.authorComastri, A.-
dc.contributor.authorDadina, M.-
dc.contributor.authorLanzuisi, G.-
dc.contributor.authorMainieri, V.-
dc.contributor.authorMingozzi, M.-
dc.contributor.authorPerna, M.-
dc.contributor.authorVenturi, G.-
dc.contributor.authorVignali, C.-
dc.date.accessioned2022-02-15T14:12:43Z-
dc.date.available2022-02-15T14:12:43Z-
dc.date.issued2021-04-20-
dc.identifier.citationAstronomy and Astrophysics 648: A99(2021)es
dc.identifier.issn0004-6361-
dc.identifier.otherhttps://www.aanda.org/articles/aa/abs/2021/04/aa40190-20/aa40190-20.html-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/573-
dc.description.abstractAims. Outflows driven by active galactic nuclei (AGN) are expected to have a significant impact on host galaxy evolution, but the matter of how they are accelerated and propagated on galaxy-wide scales is still under debate. This work addresses these questions by studying the link between X-ray, nuclear ultra-fast outflows (UFOs), and extended ionised outflows, for the first time, in two quasars close to the peak of AGN activity (z ∼ 2), where AGN feedback is expected to be more effective. Methods. Our selected targets, HS 0810+2554 and SDSS J1353+1138, are two multiple-lensed quasars at z ∼ 1.5 with UFO detection that have been observed with the near-IR integral field spectrometer SINFONI at the VLT. We performed a kinematical analysis of the [O III]λ5007 optical emission line to trace the presence of ionised outflows. Results. We detected spatially resolved ionised outflows in both galaxies, extended more than 8 kpc and moving up to v > 2000 km s−1. We derived mass outflow rates of ∼12 M⊙ yr−1 and ∼2 M⊙ yr−1 for HS 0810+2554 and SDSS J1353+1138. Conclusions. Compared with the co-hosted UFO energetics, the ionised outflow energetics in HS 0810+2554 is broadly consistent with a momentum-driven regime of wind propagation, whereas in SDSS J1353+1138, it differs by about two orders of magnitude from theoretical predictions, requiring either a massive molecular outflow or a high variability of the AGN activity to account for such a discrepancy. By additionally considering our results together with those from the small sample of well-studied objects (all local but one) having both UFO and extended (ionised, atomic, or molecular) outflow detections, we found that in 10 out of 12 galaxies, the large-scale outflow energetics is consistent with the theoretical predictions of either a momentum- or an energy-driven scenario of wind propagation. This suggests that such models explain the acceleration mechanism of AGN-driven winds on large scales relatively well.es
dc.description.sponsorshipWe thank the anonymous referee for comments and suggestions, which have improved the paper. We acknowledge support from the Italian Ministry for University and Research (MUR) for the BLACKOUT project funded through grant PRIN 2017PH3WAT.003. MP is supported by the Programa Atraccion de Talento de la Comunidad de Madrid via grant 2018-T2/TIC11715. MP acknowledges support from the Spanish Ministerio de Economia y Competitividad through the grant ESP2017-83197-P, and PID2019-106280GB-I00. Some data shown in this work were obtained from the Mikulski Archive for Space Telescopes (MAST).es
dc.language.isoenges
dc.publisherEDP Scienceses
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2017-83197-P-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-106280GB-I00/ES/PARTICIPACION ESPAÑOLA EN EL TELESCOPIO JAMES WEBB: ACTIVIDADES PREVIAS AL LANZAMIENTO, CARACTERIZACION EN ORBITA,Y PREPARACION DE PROGRAMAS CIENTIFICOS DE TIEMPO GARANTIZADO/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.subjectGalaxies: evolutiones
dc.subjectQuasars: emission lineses
dc.subjectISM: jets and outflowses
dc.subjectTechniques: imaging spectroscopyes
dc.subjectGalaxies: activees
dc.titleConnecting X-ray nuclear winds with galaxy-scale ionised outflows in two z  ∼  1.5 lensed quasarses
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidTozzi, G. [0000-0003-4226-7777]-
dc.contributor.orcidCresci, G. [0000-0002-5281-1417]-
dc.contributor.orcidMarasco, A. [0000-0002-5655-6054]-
dc.contributor.orcidNardini, E. [0000-0001-9226-8992]-
dc.contributor.orcidMarconi, A. [0000-0002-9889-4238]-
dc.contributor.orcidMannucci, F. [0000-0002-4803-2381]-
dc.contributor.orcidRizzo, F. [0000-0001-9705-2461]-
dc.contributor.orcidAmiri, A. [0000-0002-8553-1964]-
dc.contributor.orcidDadina, M. [0000-0002-7858-7564]-
dc.contributor.orcidLanzuisi, G. [0000-0001-9094-0984]-
dc.contributor.orcidMainieri, V. [0000-0002-1047-9583]-
dc.contributor.orcidMingozzi, M. [0000-0003-2589-762X]-
dc.contributor.orcidPerna, M. [0000-0002-0362-5941]-
dc.contributor.orcidVenturi, G. [0000-0001-8349-3055]-
dc.identifier.doi10.1051/0004-6361/202040190-
dc.identifier.e-issn1432-0746-
dc.contributor.funderItalian Ministry for University and Research (MUR)-
dc.contributor.funderAgencia Estatal de Investigación (AEI)-
dc.contributor.funderComunidad de Madrid-
dc.description.peerreviewedPeerreviewes
dc.identifier.funderhttp://dx.doi.org/10.13039/501100011033-
dc.identifier.funderhttp://dx.doi.org/10.13039/100012818-
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
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