J/MNRAS/392/768ivo://CDS.VizieR/J/MNRAS/392/768doi:10.26093/cds/vizier.73920768CDSHill T.Pinte C.Minier V.Burton M.G.Cunningham M.R.2024-07-08T20:15:11Z2010-07-09T10:00:19ZCDS support team

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

cds-question@unistra.frmillimeter-astronomysubmillimeter-astronomyastrophysical-masersradio-astronomyh-ii-regionsspectral-energy-distributionConcatenating data from the millimetre regime to the infrared, we have performed spectral energy distribution (SED) modelling for 227 of the 405 millimetre continuum sources of Hill et al. (2005, Cat. J/MNRAS/363/405) which are thought to contain young massive stars in the earliest stages of their formation. Three main parameters are extracted from the fits: temperature, mass and luminosity. The method employed was the Bayesian inference, which allows a statistically probable range of suitable values for each parameter to be drawn for each individual protostellar candidate. This is the first application of this method to massive star formation.2009MNRAS.392..768Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/392/768CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/363/405 : SIMBA observations of cold cores (Hill+, 2005)J/MNRAS/368/1223 : SCUBA observations of cold cores (Hill+, 2006)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/392/768https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/392/768http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/392/768https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/392/768https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/392/768http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/392/768GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/392/768/table2 (*Parameters resulting from SED modelling of 180 of the 405 sources in the SIMBA source list)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/392/768/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/392/768/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/392/768/table2?GETtext/xml+votable180.050000true91.942875-6.38472220.0055555555555555566/14353 21458 24325 28829-28831 28890 28896 28912-28913 28918-28919 29070 29090-29092 29094 29096-29097 29099-29101 29103 29114-29116 29160 29461 29505 29510-29511 29529 29532-29533 29535 30218-30219 30241 30256 30259 30262-30263 30268-30269 30312-30313 30318-30319 30405 30420 37244 37839 37846 37897 37938 38020 41653 41655 41804 42159 43013 43024 43041https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/392/768?format=asciiRadiodefaultJ/MNRAS/392/768/table2*Parameters resulting from SED modelling of 180 of the 405 sources in the SIMBA source listrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Peak right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Peak declination (J2000)pos.eq.dec;meta.main[HBM2005]Source name (GLLL.ll+BB.BBBA) (1)meta.id;meta.maincharn_[HBM2005][*] * = Sources which have a distance ambiguitymeta.notecharTr[mr ] Ident tracer (2)meta.codecharFitFit type, Single or SED (3)stat.fit.param;meta.modelledcharn_Fit[*] * = sources that were fit with IRAS upper limitsmeta.notecharTminMinimum cold temperatureKphys.temperaturefloatTmaxMaximum cold temperatureKphys.temperaturefloatMminMinimum masssolMassphys.massdoubleMmaxMaximum masssolMassphys.massdoubleLmimMinimum luminositysolLumphys.luminositydoubleLmaxMaximum luminositysolLumphys.luminositydouble