J/A+A/614/A94ivo://CDS.VizieR/J/A+A/614/A94doi:10.26093/cds/vizier.36140094CDSHumire P.K.Neil N.M.Finlez C.Firpo V.Slater R.Lena D.Soto P.R.,Munoz D.Riel R.Schmitt H.R.Kraemer S.B.Schnorr-Mueller A.,Fischer T.C.Robinson A.Storchi-Bergmann T.Crenshaw M.Elvis M.S2018-09-18T15:24:07Z2018-06-21T08:22:25ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frseyfert-galaxiesspectrophotometryvisible-astronomyWe present two-dimensional stellar and gaseous kinematics of the inner 0.7x1.2kpc^2^ of the Seyfert 1.5 galaxy ESO 362-G18, derived from optical (4092-7338{AA}) spectra obtained with the GMOS integral field spectrograph on the Gemini South telescope at a spatial resolution of 170 pc and spectral resolution of 36km/s. ESO 362-G18 is a strongly perturbed galaxy of morphological type Sa or S0/a, with a minor merger approaching along the NE direction. Previous studies have shown that the [OIII] emission shows a fan-shaped extension of ~10" to the SE. We detect the [OIII] doublet, [NII] and H{alpha} emission lines throughout our FOV. The stellar kinematics is dominated by circular motions in the galaxy plane, with a kinematic position angle of ~137{deg} and is centred approximately on the continuum peak. The gas kinematics is also dominated by rotation, with kinematic position angles ranging from 122{deg} to 139{deg}, projected velocity amplitudes of the order of 100km/s, and a mean velocity dispersion of 100km/s. A double-Gaussian fit to the [OIII]{lambda}5007 and H{alpha} lines, which have the highest signal to noise ratios of the emission lines, reveal two kinematic components: (1) a component at lower radial velocities which we interpret as gas rotating in the galactic disk; and (2) a component with line of sight (LOS) velocities 100-250km/s higher than the systemic velocity, interpreted as originating in the outflowing gas within the AGN ionization cone. We estimate a mass outflow rate of 7.4x10^-2^M_{sun}_/yr in the SE ionization cone (this rate doubles if we assume a biconical configuration), and a mass accretion rate on the supermassive black hole (SMBH) of 2.2x10^-2^M_{sun}_/yr. The total ionized gas mass within 84pc of the nucleus is 3.3x10^5^M_{sun}_; infall velocities of ~34km/s in this gas would be required to feed both the outflow and SMBH accretion.2018A&A...614A..94Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/614/A94CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/614/A94https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/614/A94http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/614/A94https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/614/A94https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/614/A94http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/614/A94GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/614/A94/list (Informations on fits datacube)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/614/A94/list?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/614/A94/list?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/614/A94/list?GETtext/xml+votable180.050000true79.89921-32.657780.0055555555555555566/34294https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/614/A94?format=asciiOpticaldefaultJ/A+A/614/A94/listInformations on fits datacubeDEJ2000Declination of center (J2000)degpos.eq.dec;meta.mainrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right Ascension of center (J2000)degpos.eq.ra;meta.mainNxNumber of pixels along X-axismeta.numberintNyNumber of pixels along Y-axismeta.numberintNzNumber of slicesmeta.numberintblambdaLower value of wavelength interval0.1nmem.wlfloatBlambdaUpper value of wavelength interval0.1nmem.wlfloatdlambdaWavelength resolution0.1nmspect.resolutiondoublesizeSize of FITS fileKibytephys.size;meta.fitsintFileNameName of FITS file, in subdirectory fitsmeta.id;meta.fitscharTitleTitle of the FITS filemeta.title;meta.fitschar