J/MNRAS/403/2012ivo://CDS.VizieR/J/MNRAS/403/2012doi:10.26093/cds/vizier.74032012CDSMartin-Manjon M.L.Garcia-Vargas M.L.Molla M.Diaz A.I.2024-07-10T20:17:38Z2010-06-21T10:34:09ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsh-ii-regionschemical-abundancesThis is the second paper of a series reporting the results from the popstar evolutionary synthesis models. Here, we present synthetic emission-line spectra of HII regions photoionized by young star clusters, for seven values of cluster masses and for ages between 0.1 and 5.2Myr. The ionizing spectral energy distributions (SEDs) are those obtained by the popstar code for six different metallicities, with a very low-metallicity set, Z=0.0001 , not included in previous similar works. We assume that the radius of the HII region is the distance at which the ionized gas is deposited by the action of the mechanical energy of the winds and supernovae from the central ionizing young cluster.2010MNRAS.403.2012Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/403/2012CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/MNRAS/398/451 : PopStar I: Evolutionary synthesis models (Molla+, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/403/2012https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/403/2012http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/403/2012https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/403/2012https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/403/2012http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/403/2012GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/403/2012/table1AbundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElementphys.atmol.elementcharSolSolar abundances (1)phys.abundfloatDeplDepleted solar abundances (1)phys.abundfloatZ0001Abundances for Z=0.0001 (1)phys.abundfloatZ0004Abundances for Z=0.0004 (1)phys.abundfloatZ004Abundances for Z=0.004 (1)phys.abundfloatZ008Abundances for Z=0.008 (1)phys.abundfloatZ02Abundances for Z=0.02 (1)phys.abundfloatZ05Abundances for Z=0.05 (1)phys.abundfloatJ/MNRAS/403/2012/emlinesEmission lines intensities for the elctronic densities 10 and 100cm^-1^recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNeElectronic density (10 or 100 e^-^/cm^3^)cm**-3phys.densityintnullableZMetallicityphys.abund.ZfloatlogtAge (logarithmic scale)log(yr)time.agefloatMassMass of the clustersolMassphys.massdouble[OII]Normalized line intensity for [OII]3727 (1)spect.line.intensity;arith.ratiofloat[OIII]aNormalized line intensity for [OIII]5007 (1)spect.line.intensity;arith.ratiofloat[OIII]bNormalized line intensity for [OIII]4959 (1)spect.line.intensity;arith.ratiofloat[OIII]cNormalized line intensity for [OIII]4363 (1)spect.line.intensity;arith.ratiofloat[OI]Normalized line intensity for [OI]6300 (1)spect.line.intensity;arith.ratiofloat[NII]aNormalized line intensity for [NII]6584 (1)spect.line.intensity;arith.ratiofloat[NII]bNormalized line intensity for [NII]6548 (1)spect.line.intensity;arith.ratiofloat[SII]Normalized line intensity for [SII]6716 (1)spect.line.intensity;arith.ratiofloat[SIII]aNormalized line intensity for [SIII]6731 (1)spect.line.intensity;arith.ratiofloat[SIII]bNormalized line intensity for [SIII]6312 (1)spect.line.intensity;arith.ratiofloat[SIII]cNormalized line intensity for [SIII]9069 (1)spect.line.intensity;arith.ratiofloat[SIII]dNormalized line intensity for [SIII]9532 (1)spect.line.intensity;arith.ratiofloat[NeIII]Normalized line intensity for [NeIII]3869 (1)spect.line.intensity;arith.ratiofloat[HeI]aNormalized line intensity for [HeI]4471 (1)spect.line.intensity;arith.ratiofloat[HeI]bNormalized line intensity for [HeI]5871 (1)spect.line.intensity;arith.ratiofloat[HeII]Normalized line intensity for [HeII]4686 (1)spect.line.intensity;arith.ratiofloat[Ha]Normalized line intensity for [Ha] (1)spect.line.intensity;arith.ratiofloat[Hb]Line intensity for Hbeta in logarithmic scale (ergs/s)log(1e-07W)spect.line.intensityfloatlogUIonization parameter in logarithmic scaleinstr.scalefloatRadRadius of the HII regionpcphys.size.radius;obs.fielddouble