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<ri:Resource created="2025-02-18T14:44:08Z" status="active" updated="2025-07-18T20:17:17Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Neutral gas winds of MaNGA-DR15 galaxies</title><shortName>J/MNRAS/511/4223</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/511/4223</identifier><altIdentifier>doi:10.26093/cds/vizier.75114223</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Avery C.R.</name></creator><creator><name>Wuyts S.</name></creator><creator><name>Forster Schreiber N.M.</name></creator><creator><name>Villforth C.</name></creator><creator><name>Bertemes C.,Hamer S.L.</name></creator><creator><name>Sharma R.</name></creator><creator><name>Toshikawa J.</name></creator><creator><name>Zhang J.</name></creator><date role="Updated">2025-07-18T20:17:17Z</date><date role="Created">2025-02-18T14:44:08Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>star-forming-regions</subject><subject>interstellar-medium</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>redshifted</subject><subject>galaxy-radii</subject><subject>active-galactic-nuclei</subject><subject>radial-velocity</subject><subject>stellar-mass-loss</subject><description>This paper investigates the neutral gas phase of galactic winds via the Na I D{lambda}{lambda}5890, 5895{AA} feature within z ~ 0.04 MaNGA galaxies and directly compares their incidence and strength to the ionized winds detected within the same parent sample. We find evidence for neutral outflows in 127 galaxies (~5 per cent of the analysed line-emitting sample). Na I D winds are preferentially seen in galaxies with dustier central regions and both wind phases are more often found in systems with elevated star formation rate (SFR) surface densities, especially when there has been a recent upturn in the star formation activity according to the SFR_5Myr_ / SFR_800Myr_ parameter. We find the ionized outflow kinematics to be in line with what we measure in the neutral phase. This demonstrates that, despite their small contributions to the total outflow mass budget, there is value to collecting empirical measurements of the ionized wind phase to provide information on bulk motion in the outflow. Depending on dust corrections applied to the ionized gas diagnostics, the neutral phase has ~1.2-1.8 dex higher mass outflow rates (dM/dt_out_), on average, compared to the ionized phase. We quantify scaling relations between dM/dt_out_ and the strengths of the physical wind drivers (SFR, L_AGN_). Using a radial-azimuthal stacking method, and by considering inclination dependencies, we find results consistent with biconical outflows orthogonal to the disc plane. Our work complements other multiphase outflow studies in the literature that consider smaller samples, more extreme objects, or proceed via stacking of larger samples.</description><source format="bibcode">2022MNRAS.511.4223A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/511/4223</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/623/A171">J/A+A/623/A171 : Mkn 848 MaNGA 3-D data cube (Perna+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/883/175">J/ApJ/883/175 : First release of the MaNGA Stellar Library 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>MaNGAId</name><description>Identifier for MaNGA galaxy (MaNGAId)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>z</name><description>Spectrscopic redshifts (z)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logRe</name><description>Logarithm of the effective radii quantified on the NASA-Sloan Atlas r-band images are taken directly from MaNGA DR15 (logR_e_)</description><unit>log(kpc)</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>i</name><description>? 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