000096829 001__ 96829
000096829 005__ 20201124104757.0
000096829 0247_ $$2doi$$a10.1051/0004-6361/201935283
000096829 0248_ $$2sideral$$a113199
000096829 037__ $$aART-2019-113199
000096829 041__ $$aeng
000096829 100__ $$aHusemann, B.
000096829 245__ $$aThe Close AGN Reference Survey (CARS): A massive multi-phase outflow impacting the edge-on galaxy HE 1353-1917
000096829 260__ $$c2019
000096829 5060_ $$aAccess copy available to the general public$$fUnrestricted
000096829 5203_ $$aContext. Galaxy-wide outflows driven by star formation and/or an active galactic nucleus (AGN) are thought to play a crucial rule in the evolution of galaxies and the metal enrichment of the inter-galactic medium. Direct measurements of these processes are still scarce and new observations are needed to reveal the nature of outflows in the majority of the galaxy population. 
Aims. We combine extensive, spatially-resolved, multi-wavelength observations, taken as part of the Close AGN Reference Survey (CARS), for the edge-on disc galaxy HE 1353-1917 in order to characterise the impact of the AGN on its host galaxy via outflows and radiation. 
Methods. Multi-color broad-band photometry was combined with spatially-resolved optical, near-infrared (NIR) and sub-mm and radio observations taken with the Multi-Unit Spectroscopy Explorer (MUSE), the Near-infrared Integral Field Spectrometer (NIFS), the Atacama Large Millimeter Array (ALMA), and the Karl G. Jansky Very Large Array (VLA) to map the physical properties and kinematics of the multi-phase interstellar medium. 
Results. We detect a biconical extended narrow-line region ionised by the luminous AGN orientated nearly parallel to the galaxy disc, extending out to at least 25 kpc. The extra-planar gas originates from galactic fountains initiated by star formation processes in the disc, rather than an AGN outflow, as shown by the kinematics and the metallicity of the gas. Nevertheless, a fast, multi-phase, AGN-driven outflow with speeds up to 1000 km s(-1) is detected close to the nucleus at 1 kpc distance. A radio jet, in connection with the AGN radiation field, is likely responsible for driving the outflow as confirmed by the energetics and the spatial alignment of the jet and multi-phase outflow. Evidence for negative AGN feedback suppressing the star formation rate (SFR) is mild and restricted to the central kpc. But while any SFR suppression must have happened recently, the outflow has the potential to greatly impact the future evolution of the galaxy disc due to its geometrical orientation. 
Conclusions. Our observations reveal that low-power radio jets can play a major role in driving fast, multi-phase, galaxy-scale outflows even in radio-quiet AGN. Since the outflow energetics for HE 1353-1917 are consistent with literature, scaling relation of AGN-driven outflows the contribution of radio jets as the driving mechanisms still needs to be systematically explored.
000096829 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/
000096829 590__ $$a5.636$$b2019
000096829 591__ $$aASTRONOMY & ASTROPHYSICS$$b11 / 68 = 0.162$$c2019$$dQ1$$eT1
000096829 592__ $$a2.174$$b2019
000096829 593__ $$aSpace and Planetary Science$$c2019$$dQ1
000096829 593__ $$aAstronomy and Astrophysics$$c2019$$dQ1
000096829 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000096829 700__ $$aScharwachter, J.
000096829 700__ $$aDavis, T.A.
000096829 700__ $$0(orcid)0000-0001-5654-0266$$aPerez-Torres, M.$$uUniversidad de Zaragoza
000096829 700__ $$aSmirnova-Pinchukova, I.
000096829 700__ $$aTremblay, G.R.
000096829 700__ $$aKrumpe, M.
000096829 700__ $$aCombes, F.
000096829 700__ $$aBaum, S.A.
000096829 700__ $$aBusch, G.
000096829 700__ $$aConnor, T.
000096829 700__ $$aCroom, S.M.
000096829 700__ $$aGaspari, M.
000096829 700__ $$aKraft, R.P.
000096829 700__ $$aO'Dea, C.P.
000096829 700__ $$aPowel, M.
000096829 700__ $$aSingha, M.
000096829 700__ $$aUrrutia, T.
000096829 7102_ $$12004$$2038$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Astronomía y Astrofísica
000096829 773__ $$g627 (2019), A53 [28 pp]$$pAstron. astrophys.$$tAstronomy & astrophysics$$x0004-6361
000096829 8564_ $$s3364590$$uhttps://zaguan.unizar.es/record/96829/files/texto_completo.pdf$$yVersión publicada
000096829 8564_ $$s577458$$uhttps://zaguan.unizar.es/record/96829/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000096829 909CO $$ooai:zaguan.unizar.es:96829$$particulos$$pdriver
000096829 951__ $$a2020-11-22-12:40:14
000096829 980__ $$aARTICLE