J/A+A/659/A131ivo://CDS.VizieR/J/A+A/659/A131doi:10.26093/cds/vizier.36590131CDSDeconto-Machado A.Riffel R.A.Ilha G.S.Rembold S.B.,Storchi-Bergmann T.Riffel R.Schimoia J.S.Schneider D.P.Bizyaev D.,Feng S.Wylezalek D.da Costa L.N.do Nascimento J.C.Maia M.A.G.2023-11-07T09:11:26Z2022-03-17T13:05:08ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiredshiftedabsolute-magnitudeFeedback from active galactic nuclei (AGN) in general seems to play an important role in the evolution of galaxies, although the impact of AGN winds on their host galaxies is still pending on detailed analysis. We analyse the kinematics of a sample of 170 AGN host galaxies as compared to those of a matched control sample of nonactive galaxies from the MaNGA survey in order to characterise and estimate the extents of the Narrow Line Region (NLR) and of the kinematically disturbed region (KDR) by the AGN. We define the observed NLR radius (r_NLR,o_) as the farthest distance from the nucleus within which both [OIII]/H{beta} and [NII]/H{alpha} ratios fall in the AGN region of the BPT diagram and the H equivalent width is required to be larger than 3.0{AA}. The extent of the KDR (rKDR,o) is defined as the distance from the nucleus within which the AGN hosts galaxies shows a more disturbed gas kinematics than the control galaxies. The AGN [OIII]5007 luminosity ranges from 10^39^ to 10^41^erg/s, and the kinematics derived from the [OIII] line profiles reveal that, on average, the most luminous AGN (L[OIII]>3.8x10^40^erg/s) possess higher residual difference between the gaseous and stellar velocities and velocities dispersion than their control galaxies in all the radial bins. Spatially resolved NLR's and KDR's were found in 55 and 46 AGN host galaxies, with corrected radii 0.2<r_KDR,c_<2.3kpc and 0.4<r_NLR,c_<10.1kpc, with a relation between the two given by logr_KDR,c_=(0.53+/-0.12)logr_NLR,c_+(1.07+/-0.22), respectively. On average, the extension of the KDR corresponds to about 30 per cent of that of the NLR. Assuming that the KDR is due to an AGN outflow, we have estimated ionised gas mass outflow rates that range between 10^-5^ and ~1M_{sun}_/yr, and kinetic powers that range from 10^34^ to 10^40^erg/s. Comparing the power of the AGN ionised outflows with the AGN luminosities, they are always below the 0.05 LAGN model threshold for having a an important feedback effect on their respective host galaxies. The mass outflow rates (and power) of our AGN sample correlate with their luminosities, populating the lowest AGN luminosity range of the correlations previously found for more powerful sources.2022A&A...659A.131Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/659/A131CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/AJ/154/86 : MaNGA catalog, DR15 (Wake+, 2017)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/659/A131https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/659/A131http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/659/A131https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/659/A131https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/659/A131http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/659/A131GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/659/A131/table1 (Properties of AGN hosts in our sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/659/A131/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/659/A131/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/659/A131/table1?GETtext/xml+votable180.050000true166.1294142.624553890.005555555555555556Cone search capability for table J/A+A/659/A131/table2 (Properties of control galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/659/A131/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/659/A131/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/659/A131/table2?GETtext/xml+votable180.050000true117.4560011134.883911110.0055555555555555566/555 4109 4123 4651 4704 4716 4718 4726 4734 4743 4747 4750-4751 4758 4767 4794 4796 4814 4822 4826 4829 4834-4835 4838 4841 4854 4910 4919 4960 4992 4994 4998 5000 5362 5470 5530 5532-5534 5551 5555-5556 5558-5559 5567 5579 5594 5600 5605 5615 5617-5618 5620-5621 5637 5639 5674 5727 5755 5789 5800 5816 5819 5824-5825 5827 5831 5890 5922 5929 5952 5954-5955 5958-5959 5967 5972 5982 6208-6209 6211-6212 6214 6219-6220 6222-6223 6226 6235-6236 6239 6243 6259-6261 6263 6270-6271 6385 6391 6396 6399 6438 6442 6447 6451 6458-6459 6521-6522 6528 6535 6539 6541 6547 6552-6553 6569 6575-6578 6581-6584 6588 6602 6605 6608 6627 6629 6633 6637 6643 6649 6742 7184 7186 7232 7307 7311 7318-7319 7328 7339 7341 7354 7368-7370 7680 7696 8567 8574 8661 8685 8695 8700-8702 8890 8894 9029 9039 9050 9069 9084 9116 9161 9166 9242 9252 9255-9256 9258-9259 9261 9265 9267 9272 9279 9310 9341 9344 9346 9353-9354 9356 9359 9367 9370 9400 9416 9418 9462 9467-9468 9470-9471 9474 9480 9484 9505 9511-9512 9604-9606 9632-9634 9638 9640 9642-9644 9646 9785 9788 9799 9807 9811 9814 9817 9828-9830 9833 9837 9839 9848 9850-9851 9898 9901 9906 9909 9911 9922 9928 9937 9942-9943 9958 9984 9986-9987 9990 9992-9993 10022 10085-10086 10099 10104 10112 10120 10181-10183 10192 10200-10202 10213 10247 10259 10263 10267 10269-10271 10289-10290 10292 10294-10295 10297 10304 10374 10377-10378 10380 10390 10393 10399 10437 10456 10487 10556 10602 10622 10644 10654 10662 10677 10691 10695-10696 10701 10712 10746 10775 10795-10796 10866 10869 10872 10880 10893 10911 10924 10934 10936 10954 10960 10978 10998-10999 11004 11023 11033 11043-11044 11079 11090 11268 11288 11301 11312-11313 11323 11348 11357 11380-11381 11403 11407 11409 11412 11430 11593 12383 12390 12399 17745 17747 17750 17753 17756 17776 18070 18302 19099 19116 19426 21887 23045 23057 23101-23103 23183 23187 23192 23194 23202 23205 23208-23210 23216 27259 27314 27337 27348 28151 28269 28271 28280 28282 28340 28361 28366 28369 28636 30036 30040-30041 32486 32509 32681 36717https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/659/A131?format=asciidefaultJ/A+A/659/A131/table1Properties of AGN hosts in our samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAGNIdentification of the AGN host in the MaNGA survey (1)meta.id;meta.maincharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainzSDSS-III spectroscopic redshiftsrc.redshiftfloatrMAGSDSS-III integrated r-band absolute magnitudemagphys.magAbsfloatlogM*? Logarithmic stellar masslog(solMass)phys.massfloatnullableClassGalaxy Zoo I morphological classificationsrc.morphcharL[OIII]Luminosity of [OIII] 5007{AA} line from SDSS-III spectra1e+33Wphys.luminosityfloate_L[OIII]Error on luminosity of [OIII] 5007{AA} line from SDSS-III spectra1e+33Wstat.errorfloatSimbadSimbad column added by the CDSmeta.ref.urlcharJ/A+A/659/A131/table2Properties of control galaxiesDEJ2000Control galaxy Declination (J2000)degpos.eq.dec;meta.mainzSDSS-III spectroscopic redshiftsrc.redshiftfloatrMAGSDSS-III integrated r-band absolute magnitudemagphys.magAbsfloatlogM*logarithmic stellar masslog(solMass)phys.massfloatClassGalaxy Zoo I morphological classificationsrc.morphcharL[OIII]Luminosity of [OIII] 5007{AA} line from SDSS-III spectra1e+33Wphys.luminosityfloate_L[OIII]Error on luminosity of [OIII] 5007{AA} line from SDSS-III spectra1e+33Wstat.errorfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAGNIdentification of the AGN host in the MaNGA survey (1)meta.id;meta.maincharControlIdentification of the control galaxies associated to the AGN hostmeta.idcharRAJ2000Control galaxy Right ascension (J2000)degpos.eq.ra;meta.mainSimbadSimbad column added by the CDSmeta.ref.urlchar