J/A+AS/119/111ivo://CDS.VizieR/J/A+AS/119/111CDSLee H.-H.Bettens R.P.A.Herbst E.2004-08-23T08:46:05Z2004-08-23T08:45:45ZCDS support team

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

cds-question@unistra.frinterstellar-mediumchemical-abundancesIn this paper we present calculated fractional abundances in dense interstellar clouds for selected atomic and molecular species using three different homogeneous, pseudo-time-dependent models discussed by Bettens, Lee, & Herbst (1995): the new standard model, the new neutral-neutral model, and model 4. We have run each model with 3 different hydrogen densities - 1,000; 10,000; and 100,000cm-3 - and two temperatures - 10K and 50K. "Low metal" elemental abundances have been used for all three models; the new standard model has also been run with "high metal" abundances.1996A&AS..119..111Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/119/111CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/119/111https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/119/111http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/119/111https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/119/111https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/119/111http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/119/111GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+AS/119/111/standardNew standard model (tables 2,3,4)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnH[1.e3,1.e5] Densitycm**-3phys.densityfloatT[10,50] Cloud temperatureKphys.temperatureintSpeciesSpecies namemeta.id;phys.molcharA4.5Fractional abundances at 10+4.5 yearsphys.abunddoubleA5Fractional abundances at 10+5 yearsphys.abunddoubleA5.5Fractional abundances at 10+5.5 yearsphys.abunddoubleAstsFractional abundances at steady statephys.abunddoubleJ/A+AS/119/111/neu_neuNew neutral-neutral model (tables 5,6,7)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnH[1.e3,1.e5] Densitycm**-3phys.densityfloatT[10,50] Cloud temperatureKphys.temperatureintSpeciesSpecies namemeta.id;phys.molcharA4.5Fractional abundances at 10+4.5 yearsphys.abunddoubleA5Fractional abundances at 10+5 yearsphys.abunddoubleA5.5Fractional abundances at 10+5.5 yearsphys.abunddoubleAstsFractional abundances at steady statephys.abunddoubleJ/A+AS/119/111/model4Model4 (Bettens 1995ApJ...443..664B) tables 8,9,10recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnH[1.e3,1.e5] Densitycm**-3phys.densityfloatT[10,50] Cloud temperatureKphys.temperatureintSpeciesSpecies namemeta.id;phys.molcharA4.5Fractional abundances at 10+4.5 yearsphys.abunddoubleA5Fractional abundances at 10+5 yearsphys.abunddoubleA5.5Fractional abundances at 10+5.5 yearsphys.abunddoubleAstsFractional abundances at steady statephys.abunddoubleJ/A+AS/119/111/high_metNew standard model(high metal) (tables 11,12,13)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnH[1.e3,1.e5] Densitycm**-3phys.densityfloatT[10,50] Cloud temperatureKphys.temperatureintSpeciesSpecies namemeta.id;phys.molcharA4.5Fractional abundances at 10+4.5 yearsphys.abunddoubleA5Fractional abundances at 10+5 yearsphys.abunddoubleA5.5Fractional abundances at 10+5.5 yearsphys.abunddoubleAstsFractional abundances at steady statephys.abunddouble