000079751 001__ 79751
000079751 005__ 20200716101454.0
000079751 0247_ $$2doi$$a10.1051/0004-6361/201935577
000079751 0248_ $$2sideral$$a112657
000079751 037__ $$aART-2019-112657
000079751 041__ $$aeng
000079751 100__ $$aSmirnova-Pinchukova, I.
000079751 245__ $$aThe Close AGN Reference Survey (CARS) Discovery of a global [C II] 158 mu m line excess in AGN HE 1353-1917
000079751 260__ $$c2019
000079751 5060_ $$aAccess copy available to the general public$$fUnrestricted
000079751 5203_ $$aThe [C II]lambda 158 mu m line is one of the strongest far-infrared (FIR) lines and an important coolant in the interstellar medium of galaxies that is accessible out to high redshifts. The excitation of [C II] is complex and can best be studied in detail at low redshifts. Here we report the discovery of the highest global [C II] excess with respect to the FIR luminosity in the nearby AGN host galaxy HE 1353-1917. This galaxy is exceptional among a sample of five targets because the AGN ionization cone and radio jet directly intercept the cold galactic disk. As a consequence, a massive multiphase gas outflow on kiloparsec scales is embedded in an extended narrow-line region. Because HE 1353-1917 is distinguished by these special properties from our four bright AGN, we propose that a global [C II] excess in AGN host galaxies could be a direct signature of a multiphase AGN-driven outflow with a high mass-loading factor.
000079751 540__ $$9info:eu-repo/semantics/openAccess$$aby$$uhttp://creativecommons.org/licenses/by/3.0/es/
000079751 590__ $$a5.636$$b2019
000079751 591__ $$aASTRONOMY & ASTROPHYSICS$$b11 / 68 = 0.162$$c2019$$dQ1$$eT1
000079751 592__ $$a2.174$$b2019
000079751 593__ $$aSpace and Planetary Science$$c2019$$dQ1
000079751 593__ $$aAstronomy and Astrophysics$$c2019$$dQ1
000079751 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/publishedVersion
000079751 700__ $$aHusemann, B.
000079751 700__ $$aBusch, G.
000079751 700__ $$aAppleton, P.
000079751 700__ $$aBethermin, M.
000079751 700__ $$aCombes, F.
000079751 700__ $$aCroom, S.
000079751 700__ $$aDavis, T.A.
000079751 700__ $$aFischer, C.
000079751 700__ $$aGaspari, M.
000079751 700__ $$aGroves, B.
000079751 700__ $$aKlein, R.
000079751 700__ $$aO''Dea, C.P.
000079751 700__ $$0(orcid)0000-0001-5654-0266$$aPerez-Torres, M.$$uUniversidad de Zaragoza
000079751 700__ $$aScharwachter, J.
000079751 700__ $$aSingha, M.
000079751 700__ $$aTremblay, G.R.
000079751 700__ $$aUrrutia, T.
000079751 7102_ $$12004$$2038$$aUniversidad de Zaragoza$$bDpto. Física Teórica$$cÁrea Astronomía y Astrofísica
000079751 773__ $$g626 (2019), L3 [7 pp]$$pAstron. astrophys.$$tAstronomy & astrophysics$$x0004-6361
000079751 8564_ $$s9660141$$uhttps://zaguan.unizar.es/record/79751/files/texto_completo.pdf$$yVersión publicada
000079751 8564_ $$s117789$$uhttps://zaguan.unizar.es/record/79751/files/texto_completo.jpg?subformat=icon$$xicon$$yVersión publicada
000079751 909CO $$ooai:zaguan.unizar.es:79751$$particulos$$pdriver
000079751 951__ $$a2020-07-16-09:08:16
000079751 980__ $$aARTICLE