J/ApJ/910/139ivo://CDS.VizieR/J/ApJ/910/139doi:10.26093/cds/vizier.19100139CDSRevalski M.Meena B.Martinez F.Polack G.E.Crenshaw D.M.,Kraemer S.B.Collins N.R.Fischer T.C.Schmitt H.R.Schmidt J.,Maksym W.P.Rafelski M.2022-11-09T06:19:09Z2022-10-25T11:49:50ZCDS support team

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

cds-question@unistra.frseyfert-galaxiesactive-galactic-nucleivisible-astronomyspectroscopyOutflows of ionized gas driven by active galactic nuclei (AGN) may significantly impact the evolution of their host galaxies. However, determining the energetics of these outflows is difficult with spatially unresolved observations that are subject to strong global selection effects. We present part of an ongoing study using Hubble Space Telescope and Apache Point Observatory spectroscopy and imaging to derive spatially resolved mass outflow rates and energetics for narrow-line region outflows in nearby AGN that are based on multi-component photoionization models to account for spatial variations in gas ionization, density, abundances, and dust content. This expanded analysis adds Mrk 3, Mrk 78, and NGC 1068, doubling our earlier sample. We find that the outflows contain total ionized gas masses of M~10^5.5^-10^7.5^M_{sun}_ and reach peak velocities of v~800-2000km/s. The outflows reach maximum mass outflow rates of dM/dt_out_3-12M_{sun}_/yr and encompass total kinetic energies of E~10^54^-10^56^erg. The outflows extend to radial distances of r~0.1-3kpc from the nucleus, with the gas masses, outflow energetics, and radial extents positively correlated with AGN luminosity. The outflow rates are consistent with in situ ionization and acceleration where gas is radiatively driven at multiple radii. These radial variations indicate that spatially resolved observations are essential for localizing AGN feedback and determining the most accurate outflow parameters.2021ApJ...910..139Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/910/139CatalogResearchIsServedByTAP VizieR generic servicerelated-toB/hst : HST Archived Exposures Catalog (STScI, 2007)J/A+A/442/137 : HI observations of WHISP disk galaxies (Noordermeer+, 2005)J/ApJ/661/L143 : Star formation rate in Seyfert galaxies (Wang+, 2007)J/ApJ/676/184 : Peculiar motion away from the Local Void (Tully+, 2008)J/A+A/564/A125 : AGN Torus model comparison of AGN in CDFS (Buchner+, 2014)J/MNRAS/480/2302 : Extended emission-line regions of obscured AGN (Sun+, 2018)J/MNRAS/486/4290 : AGN-driven winds through IR emission. II. (Baron+, 2019)J/A+A/630/A59 : ALMA datacubes for 48 QSOs (Bischetti+, 2019)J/A+A/622/A146 : MAGNUM survey galaxies images (Mingozzi+, 2019)J/MNRAS/492/3073 : CALIFA galaxies hosting an AGN (Lacerda+, 2020)J/ApJ/902/26 : HST opt. & H-band obs. of Cepheids in NGC4151 (Yuan+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/910/139https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/910/139http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/910/139https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/910/139https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/910/139http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/910/139GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/ApJ/910/139/table4Mrk 78 HST STIS flux-weighted average emission line ratiosrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPos[-3.2/3.2] Spatial distance from nucleus (G1)arcsecpos.angDistancefloatNe5-3426[0.5/3.2]? The [NeV] 3426{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Ne5-3426[0.29/3.2]? Uncertainty in Ne5-3426stat.errorfloatnullableO2-3727[1.5/6.8]? The [OII] 3727{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O2-3727[0.4/4.6]? Uncertainty in O2-3727stat.errorfloatnullableNe3-3869[0.58/5]? The [NeIII] 3869{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Ne3-3869[0.3/5]? Uncertainty in Ne3-3869stat.errorfloatnullableHe+Ne3[0.28/1.5]? The H{epsilon}+[NeIII]3969{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_He+Ne3[0.19/1.2]? Uncertainty in He+Ne3stat.errorfloatnullableS2-4074[0.24/0.8]? The [SII] 4074{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_S2-4074[0.13/0.8]? Uncertainty in S2-4074stat.errorfloatnullableHd[0.2/1.4]? The H{delta} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Hd[0.18/1.4]? Uncertainty in Hdstat.errorfloatnullableHg[0.28/1.1]? The H{gamma} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Hg[0.16/1]? Uncertainty in Hgstat.errorfloatnullableO3-4363[0.16/0.9]? The [OIII] 4363{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O3-4363[0.06/0.7]? Uncertainty in O3-4363stat.errorfloatnullableHe2-4686[0.14/0.7]? The HeII 4686{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullableHa[2/2.9] The H{alpha} line ratio (G2)spect.line.intensity;arith.ratiofloate_He2-4686[0.07/0.7]? Uncertainty in He2-4686stat.errorfloatnullableHb[1] The H{beta} line ratio (G2)spect.line.intensity;arith.ratiofloate_Hb[0.16/1] Uncertainty in Hbstat.errorfloatO3-4959[2/6.2] The [OIII] 4959{AA} line ratio (G2)spect.line.intensity;arith.ratiofloate_O3-4959[0.57/5.7] Uncertainty in O3-4959stat.errorfloatO3-5007[6/18] The [OIII] 5007{AA} line ratio (G2)spect.line.intensity;arith.ratiofloate_O3-5007[1.7/16] Uncertainty in O3-5007stat.errorfloatO1-6300[0.15/1.1]? The [OI] 6300{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O1-6300[0.13/1.1]? Uncertainty in O1-6300stat.errorfloatnullableO1-6363[0.09/0.11]? The [OI] 6363{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O1-6363[0.04/0.07]? Uncertainty in O1-6363stat.errorfloatnullableN2-6548[0.54/1]? The [NII] 6548{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_N2-6548[0.13/0.9]? Uncertainty in N2-6548stat.errorfloatnullablee_Ha[0.7/2.9] Uncertainty in Hastat.errorfloatN2-6584[1/2.8]? The [NII] 6584{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_N2-6584[0.38/2.7]? Uncertainty in N2-6584stat.errorfloatnullableS2-6716[0.3/1.5]? The [SII] 6716{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_S2-6716[0.1/1.5]? Uncertainty in S2-6716stat.errorfloatnullableS2-6731[0.38/2.7]? The [SII] 6731{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_S2-6731[0.12/2.7]? Uncertainty in S2-6731stat.errorfloatnullableFHb[0.04/42.6] The H{beta} line flux; erg/s/cm^2^mW.m**-2phot.fluxfloate_FHb[0.03/23] Uncertainty in FHbmW.m**-2stat.errorfloatJ/ApJ/910/139/table4aMrk 78 HST STIS observed emission line ratios from slits A-De_O3-5007[0.7/26]? Uncertainty in O3-5007 (G2)stat.errorfloatnullableO1-6300[0.15/2.4]? The [OI] 6300{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullableHa[1.59/21.1]? The H{alpha} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSlit[A-D] Slit identifiermeta.notecharPos[-3.5/3.2] Spatial distance from nucleus (G1)arcsecpos.angDistancefloatNe5-3426[0.29/2.4]? The [NeV] 3426{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Ne5-3426[0.1/2.2]? Uncertainty in Ne5-3426 (G2)stat.errorfloatnullableO1-3727[0.67/5.7]? The [OI] 3727{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O1-3727[0.1/6.2]? Uncertainty in O1-3727 (G2)stat.errorfloatnullableNe3-3869[0.3/2.3]? The [NeIII]3869{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Ne3-3869[0.1/2.3]? Uncertainty in Ne3-3869 (G2)stat.errorfloatnullableHe+Ne3[0.16/1]? The H{epsilon}+[NeIII]3969{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_He+Ne3[0.07/1.2]? Uncertainty in He+Ne3 (G2)stat.errorfloatnullableS2-4074[0.2/0.7]? The [SII] 4074{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_S2-4074[0.1/0.7]? Uncertainty in S2-4074 (G2)stat.errorfloatnullableHd[0.18/1.4]? The H{delta} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Hd[0.13/1.8]? Uncertainty in Hd (G2)stat.errorfloatnullableHg[0.2/1.2]? The H{gamma} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Hg[0.08/1.7]? Uncertainty in Hg (G2)stat.errorfloatnullableO3-4363[0.1/1.4]? The [OIII] 4363{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O3-4363[0.05/2.8]? Uncertainty in O3-4363 (G2)stat.errorfloatnullableHe2-4686[0.1/0.9]? The HeII 4686{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_He2-4686[0.06/1.1]? Uncertainty in He2-4686 (G2)stat.errorfloatnullableHb[1]? The H{beta} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_Hb[0.06/0.99]? Uncertainty in Hb (G2)stat.errorfloatnullableO3-4959[1.46/8.6]? The [OIII]4959{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O3-4959[0.24/8.6]? Uncertainty in O3-4959 (G2)stat.errorfloatnullableO3-5007[4.4/26]? The [OIII] 5007{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O1-6300[0.14/4]? Uncertainty in O1-6300 (G2)stat.errorfloatnullableO1-6363[0.23/0.6]? The [OI] 6363{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_O1-6363[0.1/0.9]? Uncertainty in O1-6363 (G2)stat.errorfloatnullableN2-6548[0.58/6.3]? The [NII] 6548{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_N2-6548[0.1/6.3]? Uncertainty in N2-6548 (G2)stat.errorfloatnullablee_Ha[0.5/21]? Uncertainty in Ha (G2)stat.errorfloatnullableN2-6584[0.96/18.5]? The [NII]6584{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_N2-6584[0.3/18.4]? Uncertainty in N2-6584 (G2)stat.errorfloatnullableS2-6716[0.48/4.2]? The [SII] 6716{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_S2-6716[0.18/3.9]? Uncertainty in S2-6716 (G2)stat.errorfloatnullableS2-6731[0.5/4.5]? The [SII] 6731{AA} line ratio (G2)spect.line.intensity;arith.ratiofloatnullablee_S2-6731[0.2/3.6]? Uncertainty in S2-6731 (G2)stat.errorfloatnullableJ/ApJ/910/139/table4bMrk 78 HST STIS reddening-corrected emission line ratios from slits A-DSlit[A-D] Slit identifiermeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPos[-3.5/3.2] Spatial distance from nucleus (G1)arcsecpos.angDistancefloatNe5-3426[0.48/4.4]? The [NeV] 3426{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_Ne5-3426[0.2/5.5]? Uncertainty in Ne5-3426 (1)stat.errorfloatnullableO1-3727[1/11.7]? The [OI] 3727{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_O1-3727[0.2/11]? Uncertainty in O1-3727 (1)stat.errorfloatnullableNe3-3869[0.4/5.1]? The [NeIII] 3869{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_Ne3-3869[0.15/7.6]? Uncertainty in Ne3-3869 (1)stat.errorfloatnullableHe+Ne3[0.2/2]? The H{epsilon}+[NeIII]3969{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_He+Ne3[0.1/1.6]? Uncertainty in He+Ne3 (1)stat.errorfloatnullableS2-4074[0.24/1.1]? The [SII] 4074{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_S2-4074[0.13/1]? Uncertainty in S2-4074 (1)stat.errorfloatnullableHd[0.2/1.4]? The H{delta} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_Hd[0.15/1.8]? Uncertainty in Hd (1)stat.errorfloatnullableHg[0.24/1.3]? The H{gamma} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_Hg[0.1/2.2]? Uncertainty in Hg (1)stat.errorfloatnullableO3-4363[0.12/1.7]? The [OIII] 4363{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_O3-4363[0.05/3.6]? Uncertainty in O3-4363 (1)stat.errorfloatnullableHe2-4686[0.1/1]? The HeII 4686{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_He2-4686[0.06/1.1]? Uncertainty in He2-4686 (1)stat.errorfloatnullableHb[1]? The H{beta} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_Hb[0.06/1]? Uncertainty in Hb (1)stat.errorfloatnullableO3-4959[1.46/8.1]? The [OIII] 4959{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_O3-4959[0.23/8.1]? Uncertainty in O3-4959 (1)stat.errorfloatnullableO3-5007[4.4/23.7]? The [OIII] 5007{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_O3-5007[0.7/23.7]? Uncertainty in O3-5007 (1)stat.errorfloatnullableO1-6300[0.1/1.5]? The [OI] 6300{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_O1-6300[0.1/2.1]? Uncertainty in O1-6300 (1)stat.errorfloatnullableO1-6363[0.09/0.5]? The [OI] 6363{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_O1-6363[0.04/0.7]? Uncertainty in O1-6363 (1)stat.errorfloatnullableN2-6548[0.4/1.2]? The [NII] 6548{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_N2-6548[0.09/1]? Uncertainty in N2-6548 (1)stat.errorfloatnullableHa[1.59/2.92]? The H{alpha} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_Ha[0.45/4]? Uncertainty in Ha (1)stat.errorfloatnullableN2-6584[0.89/3.3]? The [NII] 6584{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_N2-6584[0.27/3.5]? Uncertainty in N2-6584 (1)stat.errorfloatnullableS2-6716[0.25/1.5]? The [SII] 6716{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_S2-6716[0.1/1.8]? Uncertainty in S2-6716 (1)stat.errorfloatnullableS2-6731[0.3/2.7]? The [SII] 6731{AA} line ratio (1)spect.line.intensity;arith.ratiofloatnullablee_S2-6731[0.1/3.7]? Uncertainty in S2-6731 (1)stat.errorfloatnullableE(B-V)[0/1.9]? The (B-V) color excessmagphot.color.excessfloatnullablee_E(B-V)[0.1/0.8]? Uncertainty in E(B-V)magstat.errorfloatnullableHbc[0.03/20]? Extinction-corrected H{beta} line flux; in erg/s/cm^2^mW.m**-2phot.fluxfloatnullablee_Hbc[0.02/18]? Uncertainty in HbcmW.m**-2stat.errorfloatnullable