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<ri:Resource created="2026-09-03T15:21:29Z" status="active" updated="2026-09-03T14:23:37Z" 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>H II/nebulae and Ass* in PHANGS galaxies</title><shortName>J/MNRAS/522/2369</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/522/2369</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Scheuermann F.</name></creator><creator><name>Kreckel K.</name></creator><creator><name>Barnes A.T.</name></creator><creator><name>Belfiore F.</name></creator><creator><name>Groves B.</name></creator><creator><name>Hannon S.,Lee J.C.</name></creator><creator><name>Minsley R.</name></creator><creator><name>Rosolowsky E.</name></creator><creator><name>Bigiel F.</name></creator><creator><name>Blanc G.A.</name></creator><creator><name>Boquien M.,Dale D.A.</name></creator><creator><name>Deger S.</name></creator><creator><name>Egorov O.V.</name></creator><creator><name>Emsellem E.</name></creator><creator><name>Glover S.C.O.</name></creator><creator><name>Grasha K.,Hassani H.</name></creator><creator><name>Jeffreson S.M.R.</name></creator><creator><name>Klessen R.S.</name></creator><creator><name>Kruijssen J.M.D.</name></creator><creator><name>Larson K.L.,Leroy A.K.</name></creator><creator><name>Lopez L.A.</name></creator><creator><name>Pan H.-A.</name></creator><creator><name>Sanchez-Blazquez P.</name></creator><creator><name>Santoro F.,Schinnerer E.</name></creator><creator><name>Thilker D.A.</name></creator><creator><name>Whitmore B.C.</name></creator><creator><name>Watkins E.J.</name></creator><creator><name>Williams T.G.</name></creator><date role="Updated">2026-09-03T14:23:37Z</date><date role="Created">2026-09-03T15:21:29Z</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>h-ii-regions</subject><subject>nebulae</subject><subject>interstellar-medium</subject><subject>stellar-associations</subject><subject>spectroscopy</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>ultraviolet-astronomy</subject><subject>infrared-astronomy</subject><subject>star-forming-regions</subject><subject>line-intensities</subject><subject>chemical-abundances</subject><subject>astrometry</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><subject>extinction</subject><description>Connecting the gas in H II regions to the underlying source of the ionizing radiation can help us constrain the physical processes of stellar feedback and how H II regions evolve over time. With PHANGS-MUSE, we detect nearly 24000 H II regions across 19 galaxies and measure the physical properties of the ionized gas (e.g. metallicity, ionization parameter, and density). We use catalogues of multiscale stellar associations from PHANGS-HST to obtain constraints on the age of the ionizing sources. We construct a matched catalogue of 4177 H II regions that are clearly linked to a single ionizing association. A weak anticorrelation is observed between the association ages and the H{alpha} equivalent width EW(H{alpha}), the H{alpha}/FUV flux ratio, and the ionization parameter, logq. As all three are expected to decrease as the stellar population ages, this could indicate that we observe an evolutionary sequence. This interpretation is further supported by correlations between all three properties. Interpreting these as evolutionary tracers, we find younger nebulae to be more attenuated by dust and closer to giant molecular clouds, in line with recent models of feedback-regulated star formation. We also observe strong correlations with the local metallicity variations and all three proposed age tracers, suggestive of star formation preferentially occurring in locations of locally enhanced metallicity. Overall, EW(H{alpha}) and logq show the most consistent trends and appear to be most reliable tracers for the age of an H II region.</description><source format="bibcode">2023MNRAS.522.2369S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/522/2369</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/MNRAS/520/4902">J/MNRAS/520/4902 : The PHANGS-MUSE nebular catalogue (Groves+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/520/63">J/MNRAS/520/63 : Cl* ages, masses and extinctions of 4 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Error of EW(Ha)cor (EW_HA_corr_err)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>log(q)</name><description>? Ionization parameter logq (logq)</description><ucd>phys.ionizParam.rad</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_log(q)</name><description>? Error of log (q) (logq_err)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>D[O/H]</name><description>? Local metallicity offset {Delta} (O/H) (Delta_met_scal)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Ne</name><description>? Electron density (density)</description><unit>cm**-3</unit><ucd>phys.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_Ne</name><description>? Electron density (density_err)</description><unit>cm**-3</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>GMCsep</name><description>? Distance to nearest GMC giant molecular clouds (GMC_sep)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Santoro22</name><description>Display the PHANGS-MUSE sample HII regions catalog of Santoro et al. 2022A&amp;A...658A.188S, Cat. J/A+A/658/A188</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Groves23</name><description>Display the PHANGS-MUSE nebular catalog of Groves et al. 2023MNRAS.520.4902G, Cat. J/MNRAS/520/4902</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Galaxy</name><description>Name of the galaxy (gal_name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Overlap</name><description>Flag for overlap isolated, partial, contain (overlap)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Envir</name><description>Galactic environment e.g. bar, centre, and disc (environment)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column></table><table><name>J/MNRAS/522/2369/nebulae</name><description>Spectroscopic EW and luminosity Ha and Hb of detected nebulae in 19 PHANGS-MUSE galaxies</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Region</name><description>ID of the H II region (region_ID)</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAJ2000</name><description>Right ascension of the nebulae (J2000) (ra)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>indexed</flag></column><column><name>DEJ2000</name><description>Declination of the nebulae (J2000) (dec)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>indexed</flag></column><column><name>LHa</name><description>? The H{alpha} luminosity (HA)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LHa</name><description>? Error of LHa (HA_err)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>LHacont</name><description>The H{alpha} continuum luminosity (continuum_HA)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_LHacont</name><description>Error of LHacont (continuum_HA_err)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LHabkg</name><description>? The H{alpha} background continuum luminosity (continuum_HA_bkg)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.line.Halpha</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LHabkg</name><description>? Error of LHabkg (continuum_HA_bkg_err)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EW(Ha)</name><description>? The H{alpha} equivalent width (EW_HA)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_EW(Ha)</name><description>? Error of EW (Ha) (EW_HA_err)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EW(Ha)cor</name><description>? Background corrected EW (Halpha) (EW_HA_corr)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_EW(Ha)cor</name><description>? Error of EW(Ha)cor (EW_HA_corr_err)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>LHb</name><description>? The H{beta} luminosity (HB)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LHb</name><description>? Error of LHb (HB_err)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>LHbcont</name><description>The H{beta} continuum luminosity (continuum_HB)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_LHbcont</name><description>Error of LHbcont (continuum_HB_err)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LHbbkg</name><description>? The H{beta} background continuum luminosity (continuum_HB_bkg)</description><unit>1e-07W</unit><ucd>phys.luminosity;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_LHbbkg</name><description>? Error of LHbbkg (continuum_HB_bkg_err)</description><unit>1e-07W</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EW(Hb)</name><description>? The H{beta} equivalent width (EW_HB)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_EW(Hb)</name><description>? Error of EW (Hb) (EW_HB_err)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>EW(Hb)cor</name><description>? Background corrected EW (Hbeta) (EW_HB_corr)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_EW(Hb)cor</name><description>? Error of EW(Hb)cor (EW_HB_corr_err)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Santoro22</name><description>Display the PHANGS-MUSE sample HII regions catalog of Santoro et al. 2022A&amp;A...658A.188S, Cat. J/A+A/658/A188</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Groves23</name><description>Display the PHANGS-MUSE nebular catalog of Groves et al. 2023MNRAS.520.4902G, Cat. J/MNRAS/520/4902</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Galaxy</name><description>Name of the galaxy (gal_name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Tmatched</name><description>Link to matched.dat</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>