J/MNRAS/471/1743ivo://CDS.VizieR/J/MNRAS/471/1743doi:10.26093/cds/vizier.74711743CDSDe Vis P.Gomez H.L.Schofield S.P.Maddox S.Dunne L.Baes M.,Cigan P.Clark C.J.R.Gomez E.L.Lara-lopez M.Owers M.2024-08-17T20:20:14Z2020-07-03T14:46:28ZCDS support team

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

cds-question@unistra.frgalaxieschemical-abundancesspectroscopyWe combine samples of nearby galaxies with Herschel photometry selected on their dust, metal, HI and stellar mass content, and compare these to chemical evolution models in order to discriminate between different dust sources. In a companion paper, we used an HI-selected sample of nearby galaxies to reveal a subsample of very gas-rich (gas fraction >80 per cent) sources with dust masses significantly below predictions from simple chemical evolution models, and well below M_d_/M_*_ and M_d_/M_gas_ scaling relations seen in dust and stellar-selected samples of local galaxies. We use a chemical evolution model to explain these dust-poor, but gas-rich, sources as well as the observed star formation rates (SFRs) and dust-to-gas ratios. We find that (i) a delayed star formation history is required to model the observed SFRs; (ii) inflows and outflows are required to model the observed metallicities at low gas fractions; (iii) a reduced contribution of dust from supernovae (SNe) is needed to explain the dust-poor sources with high gas fractions. These dust-poor, low stellar mass galaxies require a typical core-collapse SN to produce 0.01-0.16M_{sun}_ of dust. To match the observed dust masses at lower gas fractions, significant grain growth is required to counteract the reduced contribution from dust in SNe and dust destruction from SN shocks. These findings are statistically robust, though due to intrinsic scatter it is not always possible to find one single model that successfully describes all the data. We also show that the dust-to-metal ratio decreases towards lower metallicity.2017MNRAS.471.1743Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/471/1743CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/389/845 : Spectra of blue compact galaxies (Kong+, 2002)J/A+A/448/955 : Abundances of emission galaxies in SDSS-DR3 (Izotov+, 2006)J/ApJ/662/15 : Abundances in extragalactic HII regions (Izotov+, 2007)J/A+A/464/885 : Abundances in 53 HII regions (Guseva+, 2007)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/471/1743https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/471/1743http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/471/1743https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/471/1743https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/471/1743http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/471/1743GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/471/1743/tablea1 (Basic properties for the HI-selected HiGH sample (De Vis et al., 2017MNRAS.464.4680D) and dust-selected HAPLESS sample (Clark et al., 2015, Cat. J/MNRAS/452/397))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/471/1743/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/471/1743/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/471/1743/tablea1?GETtext/xml+votable180.050000true216.72111810.96287390.005555555555555556Cone search capability for table J/MNRAS/471/1743/tablea4 (*Emission-line measurements and derived metallicities for the Dwarf Galaxy Survey (DGS, Madden et al., 2013PASP..125..600M) using the O3N2, N2, PG16S and KE08/T04 methods)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/471/1743/tablea4?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/471/1743/tablea4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/471/1743/tablea4?GETtext/xml+votable180.050000true9.2187042-33.55478610.0055555555555555565/6486 6/684 3042 3389 4105 5950 6011 6042 6046 6419 7281 7878 7946 8028 8224 10399 10431 10481 10587 10689 10769 10911 10970 11137 11177-11178 11382 18002 18198 20388 21845 21851 22828 23078 23566 24696 25591 25594-25597 25599 25659 25918 25933 25935 25958-25960 25964-25966 25970-25972 25974 25980 26049 26253-26254 26277 26279 26282 26288 26290-26291 26960 26963 26967 26969 26971 26992 27279 27650 27656 28631 29718 33986 35243 35576 36756 39602 40124 43874https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/471/1743?format=asciidefaultJ/MNRAS/471/1743/tablea1Basic properties for the HI-selected HiGH sample (De Vis et al., 2017MNRAS.464.4680D) and dust-selected HAPLESS sample (Clark et al., 2015, Cat. J/MNRAS/452/397)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/58] Sequential numbermeta.recordintNameCommon namemeta.id;meta.maincharRAdegRight ascension (J2000)degpos.eq.raDEdegDeclination (J2000)degpos.eq.decDistDistanceMpcpos.distancefloatlogM*Stellar masslog(solMass)phys.massfloatE_logM*Error on stellar mass, upper valuelog(solMass)stat.error;stat.maxfloate_logM*Error on stellar mass, lower valuelog(solMass)stat.errorfloatlogMHI? HI masslog(solMass)phys.massfloatnullablelogMdDust masslog(solMass)phys.massfloatE_logMdError on dust mass, upper valuelog(solMass)stat.error;stat.maxfloate_logMdError on dust mass, lower valuelog(solMass)stat.errorfloatlogSFRStar formation ratelog(solMass.yr**-1)phys.SFRfloatE_logSFRError on tar formation rate, upper valuelog(solMass.yr**-1)stat.error;stat.maxfloate_logSFRError on tar formation rate, lower valuelog(solMass.yr**-1)stat.error;phys.SFRfloatfg? Gas fractionphys.mass;arith.ratiofloatnullableHiGH[V-] In HiGH sample ?meta.codecharHAPLESS[V] In HAPLESS sample ?meta.codechar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/MNRAS/471/1743/tablea2Metallicity measurements in the form 12+log(O/H) for the HI-selected HiGH (De Vis et al., 2017MNRAS.464.4680D) and dust-selected HAPLESS sample (Clark et al., 2015, Cat. J/MNRAS/452/397)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/58] Sequential numbermeta.recordintNameCommon namemeta.id;meta.maincharO3N2? 12+log(O/H) abundance using O3N2 method, from Pettini & Pagel (2004MNRAS.348L..59P)phys.abundfloatnullableE_O3N2? Error on 12+log(O/H) (O3N2) abundance, upper valuestat.error;stat.maxfloatnullablee_O3N2? Error on 12+log(O/H) (O3N2) abundance, lower valuestat.errorfloatnullableN2? 12+log(O/H) abundance using N2 method, from Pettini & Pagel (2004MNRAS.348L..59P)phys.abundfloatnullableE_N2? Error on 12+log(O/H) N2 abundance, upper valuestat.error;stat.maxfloatnullablee_N2? Error on 12+log(O/H) N2 abundance, lower valuestat.errorfloatnullablePG16S? 12+log(O/H) abundance using S calibration from Pilyugin & Grebel (2016MNRAS.457.3678P)phys.abundfloatnullableE_PG16S? Error on 12+log(O/H) (PG16S) abundance, upper valuestat.error;stat.maxfloatnullablee_PG16S? Error on 12+log(O/H) (PG16S) abundance, lower valuestat.errorfloatnullableKe08/T04? 12+log(O/H) abundance using Ke08/T04 calibration (1)phys.abundfloatnullableE_Ke08/T04? Error on 12+log(O/H) (Ke08/T04) abundance, upper valuestat.error;stat.maxfloatnullablee_Ke08/T04? Error on 12+log(O/H) (Ke08/T04) abundance, lower valuestat.errorfloatnullableHiGH[V-] In HiGH sample ?meta.codecharHAPLESS[V] In HAPLESS sample ?meta.codecharJ/MNRAS/471/1743/tablea3*Emission-line measurements for the HiGH and HAPLESS samplesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/57] Sequential numbermeta.recordintNameCommon namemeta.id;meta.maincharGAMAGAMA catalogue identification numbermeta.idintCHbBalmer decrement, C(H{beta})phot.flux;arith.ratiofloatF[OII]? Stellar absorption corrected [OII] flux relative to H{beta} fluxphot.flux;arith.ratiofloatnullablee_F[OII]? Stellar absorption corrected [OII] flux relative to H{beta} flux errorstat.errorfloatnullableFHb[1] Stellar absorption corrected H{beta} flux relative to H{beta} fluxphot.flux;em.line.Hbetafloate_FHbStellar absorption corrected H{beta} flux relative to H{beta} flux errorstat.errorfloatF[OIII]1Stellar absorption corrected [OIII]4959 flux relative to H{beta} fluxphot.flux;em.line.OIII;arith.ratiofloate_F[OIII]1Stellar absorption corrected [OIII]4959 flux relative to H{beta} flux errorstat.errorfloatF[OIII]2Stellar absorption corrected [OIII]5007 flux relative to H{beta} fluxphot.flux;em.line.OIII;spect.linefloate_F[OIII]2Stellar absorption corrected [OIII]5007 flux relative to H{beta} flux errorstat.errorfloatFHaStellar absorption corrected H{alpha} flux relative to H{beta} fluxspect.line.intensity;arith.ratiofloate_FHaStellar absorption corrected H{alpha} flux relative to H{beta} flux errorstat.errorfloatF[NII]Stellar absorption corrected [NII] flux relative to H{beta} fluxphot.flux;arith.ratiofloate_F[NII]Stellar absorption corrected [NII] flux relative to H{beta} flux errorstat.errorfloatF[SII]1Stellar absorption corrected [SII]6713 flux relative to H{beta} fluxphot.flux;arith.ratiofloate_F[SII]1Stellar absorption corrected [SII]6713 flux relative to H{beta} flux errorstat.errorfloatF[SII]2? Stellar absorption corrected [SII]5731 flux relative to H{beta} fluxphot.flux;arith.ratiofloatnullablee_F[SII]2? Stellar absorption corrected [SII]5731 flux relative to H{beta} flux errorstat.errorfloatnullableOrigin[gandalf/GFC ] whether the stellar absorption-corrected fluxes were extracted using gandalf or the GFC cataloguephot.fluxcharHiGH[V-] In HiGH sample ?meta.codecharHAPLESS[V] In HARPLESS sample ?meta.codecharJ/MNRAS/471/1743/tablea4*Emission-line measurements and derived metallicities for the Dwarf Galaxy Survey (DGS, Madden et al., 2013PASP..125..600M) using the O3N2, N2, PG16S and KE08/T04 methodsSimbadNameSimbad column added by the CDSmeta.idcharNameCommon namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFHaStellar absorption corrected H{alpha} flux relative to H{beta} fluxspect.line.intensity;arith.ratiofloatF[OII]Stellar absorption corrected [OII] flux relative to H{beta} fluxphot.flux;arith.ratiofloatF[OIII]1Stellar absorption corrected [OIII]4959 flux relative to H{beta} fluxphot.flux;em.line.OIII;spect.linefloatF[OIII]2? Stellar absorption corrected [OIII]5007 flux relative to H{beta} fluxphot.flux;em.line.OIII;spect.linefloatnullableF[NII]? Stellar absorption corrected [NII] flux relative to H{beta} fluxphot.flux;arith.ratiofloatnullableF[SII]1? Stellar absorption corrected [SII]6713 flux relative to H{beta} fluxphot.flux;arith.ratiofloatnullablen_F[SII]2[a] Note on for blended [SII]6717 and [SII]6731 lines (1)meta.notecharF[SII]2? Stellar absorption corrected [SII]5731 flux relative to H{beta} fluxphot.flux;arith.ratiofloatnullableN2? 12+log(O/H) abundance using N2 method, from Pettini & Pagel (2004MNRAS.348L..59P)phys.abundfloatnullableO3N2? 12+log(O/H) abundance using O3N2 method, from Pettini & Pagel (2004MNRAS.348L..59P)phys.abundfloatnullablePG16S? 12+log(O/H) abundance using S calibration from Pilyugin & Grebel (2016MNRAS.457.3678P)phys.abundfloatnullableKe08/T04? 12+log(O/H) abundance using Ke08/T04 calibration (2)phys.abundfloatnullableRefReferences (3)meta.refchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.main