J/ApJ/779/79ivo://CDS.VizieR/J/ApJ/779/79doi:10.26093/cds/vizier.17790079CDSMa B.Tan J.C.Barnes P.J.2019-12-03T10:57:24Z2015-06-10T07:06:37ZCDS support team

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

cds-question@unistra.frmillimeter-astronomysubmillimeter-astronomysurveysgalaxy-kinematicsThe Census of High- and Medium-mass Protostars (CHaMP) is the first large-scale (280{deg}<l<300{deg}, -4{deg}<b<2{deg}), unbiased, subparsec resolution survey of Galactic molecular clumps and their embedded stars. Barnes et al. (Paper I, 2011, J/ApJS/196/12) presented the source catalog of ~300 clumps based on HCO^+^(1-0) emission, used to estimate masses M. Here we use archival midinfrared-to-millimeter continuum data to construct spectral energy distributions. Fitting two-temperature gray-body models, we derive bolometric luminosities, L. We find that the clumps have 10<~L/L_{sun}_<~10^6.5^ and 0.1<~L/M/[L_{sun}_/M_{sun}_]<~10^3^, consistent with a clump population spanning a range of instantaneous star-formation efficiencies from 0 to ~50%. We thus expect L/M to be a useful, strongly varying indicator of clump evolution during the star cluster formation process.2013ApJ...779...79Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/779/79CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/98 : MSX Infrared Astrometric Catalog (Egan+ 1996)J/ApJS/196/12 : Paper I. First results from Mopra HCO^+^ maps (Barnes+, 2011)J/ApJ/723/492 : GRS molecular clouds physical properties (Roman-Duval+, 2010)J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)J/A+A/481/345 : SED evolution in massive YSOs (Molinari+, 2008)J/MNRAS/363/405 : SIMBA observations of cold cores (Hill+, 2005)J/A+A/426/97 : SIMBA survey. 1.2-mm/IRAS sources (Faundez+, 2004)J/ApJ/566/945 : Massive star forming regions at 1.2mm (Beuther+, 2002)J/A+A/291/943 : Protostellar cores (Ossenkopf+, 1994)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/779/79https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/779/79http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/779/79https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/779/79https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/779/79http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/779/79GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/779/79/clumps (Primary and secondary physical properties of the HCO^+^(1-0) clumps (tables 2 and 3))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/779/79/clumps?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/779/79/clumps?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/779/79/clumps?GETtext/xml+votable180.050000true149.7330494-56.87575310.0055555555555555565/9480 9504 6/37333 37335 37341 37342 37343 37361 37363 37364 37366 37367 37368 37369 37371 37372 37373 37894 37897 37899 37902 37924 37926 37930 38024 38025 43017 43019 43020 43041 43043https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/779/79?format=asciiMillimeterdefaultJ/ApJ/779/79/clumpsPrimary and secondary physical properties of the HCO^+^(1-0) clumps (tables 2 and 3)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBYFThe BYF number from Paper I (Barnes et al. 2011, J/ApJS/196/12)meta.id.part;meta.mainintm_BYFSub-clump letter from Paper Imeta.id.part;meta.maincharf_BYF[*] Uncertain measurement of L (1)meta.codecharlogM[1.1/3.9] Log of the mass; from Paper I (Barnes et al. 2011, J/ApJS/196/12)log(solMass)phys.massfloatTc[14/47] Colder component temperature (2)Kphys.temperaturefloatlogF[-12/-5] Log of colder component bolometric flux; erg/s/cm^2^ (2)log(mW.m**-2)phot.flux.density;em.radiofloatlogLIR[-0.1/6.3] Log of IR luminosity (2)log(solLum)phys.luminosity;em.IRfloatlogL/M[-2/3.5] Log of IR luminosity to mass ratio (2)log(Sun)phys.luminosity;em.IRfloatTcb[10/50] Colder component temperature (3)Kphys.temperaturefloatlogFb[-12/-5] Log of colder component bolometric flux; erg/s/cm^2^ (3)log(mW.m**-2)phot.flux.density;em.radiofloatlogLIRb[-0.9/6.2] Log of IR luminosity (3)log(solLum)phys.luminosity;em.IRfloatlogL/Mb[-3/3.4] Log of IR luminosity to mass ratio (3)log(Sun)phys.luminosity;em.IRfloatlogFw[-11.5/-5.7] Log of warm component flux; erg/s/cm^2^log(mW.m**-2)phot.flux.density;em.radiofloatlogFwb[-12.2/-5.7] Log of warm component flux; (background-subtracted; in erg/s/cm^2^)log(mW.m**-2)phot.flux.density;em.radiofloatlogFIR[-14.1/-6.7]? Log of IRAC bands flux; erg/s/cm^2^log(mW.m**-2)phot.flux.density;em.IRfloatnullablelogFIRb[-13.1/-6.7]? Log of IRAC bands flux; (background-subtracted; in erg/s/cm^2^)log(mW.m**-2)phot.flux.density;em.IRfloatnullablelogIIR[-7.5/-0.8]? Log of IRAC intensity; erg/s/cm^2^/srlog(mW.m**-2.sr**-1)phot.count;em.optfloatnullablelogIIRb[-6.5/-0.6]? Log of IRAC intensity (background-subtracted; in erg/s/cm^2^/sr)log(mW.m**-2.sr**-1)phot.count;em.optfloatnullableTbol[70/259] Bolometric temperatureKphys.temperatureintTbolb[55/499] Bolometric temperature (background-subtracted)Kphys.temperatureintSigma[0.005/0.6] Mass surface density {Sigma}g.cm**-2phys.densityfloatsig.v[0.2/4.2] Velocity dispersion {sigma}_V_km/sphys.veloc.dispersionfloatalpha[1/54.4] Virial parameter {alpha}_vir_ (4)phys.mass;arith.ratiofloatlogLHCO[-0.5/2.1] Log of HCO^+^(1-0) line luminositylog(K.km.s**-1.pc**-2)phys.luminosity;em.radiofloatSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from Paper I: Barnes et al. 2011, J/ApJS/196/12 (right ascension part)degpos.eq.ra;meta.main_DEPositions from Paper I: Barnes et al. 2011, J/ApJS/196/12 (declination part)degpos.eq.dec;meta.main