J/A+AS/144/123ivo://CDS.VizieR/J/A+AS/144/123CDSWouterloot J.G.A.Heithausen A.Schreiber W.Winnewisser G2000-05-13T22:52:25Z2000-05-13T22:51:12ZCDS support team

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

cds-question@unistra.frmolecular-cloudsco-line-emissionUsing the KOSMA 3-m telescope we have made observations of the ^12^CO(J=1-0), (J=2-1) and (J=3-2), and the ^13^CO(J=1-0) and (J=2-1) transitions of the high latitude cloud MBM 32. The backend consisted of a Medium Resolution (channel width 167kHz; MRS), or a High Resolution (channel width 38.6kHz; HRS) acousto-optical Spectrometer. The following tables contain properties of clumps derived from the maps, assuming Gaussian clump parameters from the ^12^CO(J=1-0) MRS data (Table 3) ^12^CO(J=1-0) HRS data (Table 4) ^12^CO(J=2-1) MRS data (Table 5) ^13^CO(J=1-0) HRS data (Table 6). We distinguish between different velocity components.2000A&AS..144..123Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/144/123CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/144/123https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/144/123http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/144/123https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/144/123https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/144/123http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/144/123GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapRadiodefaultJ/A+AS/144/123/table3Clumps found in MBM 32 using the 12CO(J=1-0) MRS data, with TR*>0.8K, and dv'>1.0km/srecnoRecord number assigned by the VizieR team. Should Not be used for identification.intn_Vlsr[1-3] Vlsr interval (1)charoRARight ascension offset (2)arcminfloatoDEDeclination offset (2)arcminfloatVlsrLSR (Local Standard of Rest) velocity (3)km/sfloatTR*peakPeak of rms noise (T^*^_R_)Kfloatdvline widthkm/sfloatsizeGaussian FWHMpcfloatMassMasssolMassfloatnH2H2 densitycm**-3intMassvirVirial masssolMassintRemark[+-] See Note (4)charJ/A+AS/144/123/table4Clumps found in MBM 32 using the 12CO(J=1-0) HRS data, with TR*>1.4K, and dv'>0.4km/sRemark[+-] See Note (4)charrecnoRecord number assigned by the VizieR team. Should Not be used for identification.intn_Vlsr[1-3] Vlsr interval (1)charoRARight ascension offset (2)arcminfloatoDEDeclination offset (2)arcminfloatVlsrLSR (Local Standard of Rest) velocity (3)km/sfloatTR*peakPeak of rms noise (T^*^_R_)Kfloatdvline widthkm/sfloatsizeGaussian FWHMpcfloatMassMasssolMassfloatnH2H2 densitycm**-3intMassvirVirial masssolMassintJ/A+AS/144/123/table5Clumps found in MBM 32 from 12CO(J=2-1) MRS data, with TR*>0.6K, and dv'>0.6km/srecnoRecord number assigned by the VizieR team. Should Not be used for identification.intn_Vlsr[1-3] Vlsr interval (1)charoRARight ascension offset (2)arcminfloatoDEDeclination offset (2)arcminfloatVlsrLSR (Local Standard of Rest) velocity (3)km/sfloatTR*peakPeak of rms noise (T^*^_R_)Kfloatdvline widthkm/sfloatsizeGaussian FWHMpcfloatMassMasssolMassfloatnH2H2 densitycm**-3intMassvirVirial masssolMassintRemark[+-] See Note (4)charJ/A+AS/144/123/table6Clumps found in MBM 32 from 13CO(J=1-0) HRS data, with TR*>0.4K, and dv'>0.3km/srecnoRecord number assigned by the VizieR team. Should Not be used for identification.intn_Vlsr[1-3] Vlsr interval (1)charoRARight ascension offset (2)arcminfloatoDEDeclination offset (2)arcminfloatVlsrLSR (Local Standard of Rest) velocity (3)km/sfloatTR*peakPeak of rms noise (T^*^_R_)Kfloatdvline widthkm/sfloatsizeGaussian FWHMpcfloatMassMasssolMassfloatnH2H2 densitycm**-3intMassvirVirial masssolMassintRemark[+-] See Note (4)char