J/ApJ/879/131ivo://CDS.VizieR/J/ApJ/879/131doi:10.26093/cds/vizier.18790131CDSLi Z.French K.D.Zabludoff A.I.Ho L.C.2021-06-18T13:54:05Z2021-01-19T07:22:14ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesinterstellar-mediumultraviolet-photometryinfrared-photometryvisible-astronomybroad-band-photometryWe derive dust masses (M_dust_) from the spectral energy distributions of 58 post-starburst galaxies (PSBs). There is an anticorrelation between specific dust mass (M_dust_/M_*_) and the time elapsed since the starburst ended, indicating that dust was either destroyed, expelled, or rendered undetectable over the ~1Gyr after the burst. The M_dust_/M_*_ depletion timescale, 205_-37_^+58^Myr, is consistent with that of the CO-traced M_H2_/M_*_, suggesting that dust and gas are altered via the same process. Extrapolating these trends leads to the M_dust_/M_*_ and M_H2_/M_*_ values of early-type galaxies (ETGs) within 1-2Gyr, a timescale consistent with the evolution of other PSB properties into ETGs. Comparing Mdust and M_H2_ for PSBs yields a calibration, log M_H2_=0.45logM_dust_+6.02, that allows us to place 33 PSBs on the Kennicutt-Schmidt (KS) plane, {Sigma}SFR-{Sigma}M_H2_. Over the first ~200-300Myr, the PSBs evolve down and off of the KS relation, as their star formation rate (SFR) decreases more rapidly than M_H2_. Afterwards, M_H2_ continues to decline whereas the SFR levels off. These trends suggest that the star formation efficiency bottoms out at 10^-11^/yr and will rise to ETG levels within 0.5-1.1Gyr afterwards. The SFR decline after the burst is likely due to the absence of gas denser than the CO-traced H2. The mechanism of the M_dust_/M_*_ and M_H2_/M_*_ decline, whose timescale suggests active galactic nucleus/low-ionization nuclear emission-line region feedback, may also be preventing the large CO-traced molecular gas reservoirs from collapsing and forming denser star-forming clouds.2019ApJ...879..131Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/879/131CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)II/328 : AllWISE Data Release (Cutri+ 2013)V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)II/335 : Revised cat. of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)J/A+A/543/A161 : Submm obs. of 323 HRS nearby galaxies (Ciesla+, 2012)J/ApJ/745/95 : Herschel FIR & submm phot. of KINGFISH sample (Dale+, 2012)J/MNRAS/420/1684 : End of red sequence galaxies in Galaxy Zoo (Wong+, 2012)J/A+A/562/A21 : AGN feedback from CO observations (Cicone+, 2014)J/MNRAS/441/1017 : Multiwavelength photometry of 34 galaxies (Rowlands+, 2014)J/ApJS/224/38 : SPOGS. I. SDSS Shocked POststarburst Gal. (Alatalo+, 2016)J/ApJ/862/2 : Post-starburst galaxy ages from SDSS (French+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/879/131https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/879/131http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/879/131https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/879/131https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/879/131http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/879/131GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/879/131/psbgal (Post-starburst galaxies properties and archival UV-FIR photometry (Tables 1, 2, 4 and Tables 6+7 from Smercina et al. 2018ApJ...855...51S))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/879/131/psbgal?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/879/131/psbgal?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/879/131/psbgal?GETtext/xml+votable180.050000true233.1319957.882920.0055555555555555566/4504 4681 4719 4867 5121 5130 5787 5900 6087 6135 6253 6270 8398 8438 8475 8541 8615 8784 8935 9182 9228 9470 9637 9818 9980 9992 10122 10281 10298 10394 10442 10445 10891 11071 11142 11249 11376 11388 17920 18865 19110 23204 25919 26172 26961 27117 27334 27343 27456 27537 27727 27860 27915 28168 31704 31715 491123.2031150387835462e-22 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/879/131?format=asciiUVOpticalInfrareddefaultJ/ApJ/879/131/psbgalPost-starburst galaxies properties and archival UV-FIR photometry (Tables 1, 2, 4 and Tables 6+7 from Smercina et al. 2018ApJ...855...51S)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDSource identifier (G1)meta.id;meta.maincharRAJ2000[11.24/343.8] Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[-8.9/64.3] Declination (J2000)degpos.eq.dec;meta.mainFFUV[0.0005/0.63]? GALEX FUV band flux density (G2)mJyphot.flux;em.UVdoublenullablee_FFUV[0.0004/0.05]? Uncertainty in FFUV (G3)mJystat.errordoublenullableFNUV[0.003/1] GALEX NUV band flux density (G2)mJyphot.flux;em.UVdoublee_FNUV[0.0005/0.04] Uncertainty in FNFUV (G3)mJystat.errordoubleFu[0.02/2] SDSS DR14 u band flux density (G2)mJyphot.flux.density;em.opt.Udoublee_Fu[0.0018/0.11] Uncertainty in Fu (G3)mJystat.errordoubleFg[0.12/8.6] SDSS DR14 g band flux density (G2)mJyphot.flux.density;em.opt.Bdoublee_Fg[0.0015/0.3] Uncertainty in Fg (G3)mJystat.errordoubleFr[0.3/16.2] SDSS DR14 r band flux density (G2)mJyphot.flux.density;em.opt.Rdoublee_Fr[0.002/0.5] Uncertainty in Fr (G3)mJystat.errordoubleFi[0.4/22.5] SDSS DR14 i band flux density (G2)mJyphot.flux.density;em.opt.Idoublee_Fi[0.003/0.6] Uncertainty in Fi (G3)mJystat.errordoubleFz[0.58/27.6] SDSS DR14 z band flux density (G2)mJyphot.flux.density;em.opt.Idoublee_Fz[0.007/0.9] Uncertainty in Fz (G3)mJystat.errordoubleFJ[0.38/38] 2MASS J band flux density (G2)mJyphot.flux.density;em.IR.Jdoublee_FJ[0.06/2] Uncertainty in FJ (G3)mJystat.errordoubleFH[0.4/48.6] 2MASS H band flux density (G2)mJyphot.flux.density;em.IR.Hdoublee_FH[0.06/2.6] Uncertainty in FH (G3)mJystat.errordoubleFKs[0.5/38.6] 2MASS Ks band flux density (G2)mJyphot.mag;em.IR.Kdoublee_FKs[0.1/2.2] Uncertainty in FKs (G3)mJystat.errordoubleF3.4[0.4/17] AllWISE W1 (3.4um) band flux density (G2)mJyphot.mag;em.IR.3-4umfloate_F3.4[0.01/1.1] Uncertainty in F3.6 (G3)mJystat.errorfloatF4.6[0.3/10.3] AllWISE W2 (4.6um) band flux density (G2)mJyphot.mag;em.IR.4-8umfloate_F4.6[0.01/0.7] Uncertainty in F4.6 (G3)mJystat.errorfloatF12[0.8/53.5] AllWISE W3 (12um) band flux density (G2)mJyphot.flux.density;em.IR.8-15umfloate_F12[0.04/2.6] Uncertainty in F12 (G3)mJystat.errorfloatl_F22Limit flag on F22meta.code.errorcharF22[1.7/578]? AllWISE W4 (22um) band flux density (G2)mJyphot.flux.density;em.IR.15-30umfloatnullablee_F22[0.4/35]? Uncertainty in F22 (G3)mJystat.errorfloatnullableF70[7/19700]? Herschel/PACS 70 micron band flux density (G2)mJyphot.flux.density;em.IR.60-100umdoublenullablee_F70[2/1410]? Uncertainty in F70 (G3)mJystat.errorfloatnullableF100[14/18100]? Herschel/PACS 100 micron band flux density (G2)mJyphot.flux.density;em.IR.60-100umdoublenullablee_F100[2/1310]? Uncertainty in F100 (G3)mJystat.errorfloatnullableF160[6/10500]? Herschel/PACS 160 micron band flux density (G2)mJyphot.flux.density;em.mm.1500-3000GHzdoublenullablee_F160[2/755]? Uncertainty in F160 (G3)mJystat.errorfloatnullableF250[10/4150]? Herschel/SPIRE 250 micron band flux density (G2)mJyphot.flux.density;em.mm.750-1500GHzfloatnullablee_F250[4/294]? Uncertainty in F250 (G3)mJystat.errorfloatnullablel_F250Limit flag on F250meta.code.errorcharF350[10/1690]? Herschel/SPIRE 350 micron band flux density (G2)mJyphot.flux.density;em.mm.750-1500GHzfloatnullablee_F350[4/121]? Uncertainty in F350 (G3)mJystat.errorfloatnullablel_F500Limit flag on F500meta.code.errorcharF500[10/590]? Herschel/SPIRE 500 micron band flux density (G2)mJyphot.flux.density;em.mm.400-750GHzfloatnullablee_F500[5/48]? Uncertainty in F500 (G3)mJystat.errorfloatnullableSEDmeta.ref.urlcharf_ID[a] a: WISE and Herschel photometry from Smercina et al. 2018ApJ...855...51S ; data added by CDS for completeness (1)meta.codecharr50[0.96/7.41] Petrosian radius (2)arcsecphys.angSize;srcfloatlogM*[9.6/11.4] log stellar mass (3)log(solMass)phys.massfloatE_logM*[0.06/0.4] Upper uncertainty in logMlog(solMass)stat.error;stat.maxfloate_logM*[0.05/0.6] Lower uncertainty in logM*log(solMass)stat.errorfloatlogMd[5.3/9] log CIGALE-derived dust masslog(solMass)phys.massfloate_logMd[0.02/1.1] Uncertainty in logMdlog(solMass)stat.errorfloatRatio[-5/-1.8] log ratio of dust to stellar massesphys.mass;arith.ratiofloate_Ratio[0.1/1.1] Uncertainty in Ratiostat.error;arith.ratiofloatl_logMgLimit flag on logMgmeta.code.errorcharlogMg[7.7/10.1] log molecular gas mass (4)log(solMass)phys.massfloate_logMg[0.02/0.15]? Uncertainty in logMglog(solMass)stat.errorfloatnullableSFRun[0.01/28] Uncorrected star formation rate (5)log(solMass.yr**-1)meta.idfloate_SFRun[0.01/0.9] Uncertainty in SFRunlog(solMass.yr**-1)stat.errorfloatl_SFRcLimit flag on SFRcmeta.code.errorcharSFRc[0.0004/12.1]? Star formation rate corrected for AGN contributionlog(solMass.yr**-1)phys.SFRfloatnullablee_SFRc[0.01/1.3]? Uncertainty in SFRclog(solMass.yr**-1)stat.errorfloatnullableSCatDisplay data from French+, 2018, J/ApJ/862/2 and Alatalo+, 2016, J/ApJS/224/38 within 0.5"meta.ref.urlintnullableSloanDisplay the online SDSS-DR14 data for the nearest objectmeta.ref.urlchar