J/A+A/549/A130ivo://CDS.VizieR/J/A+A/549/A130doi:10.26093/cds/vizier.35490130CDSVeneziani M.Elia D.Noriega-Crespo A.Paladini R.Carey S.Faimali A.,Molinari S.Pestalozzi M.Piacentini F.E. Schisano2017-10-12T12:59:42Z2013-06-10T08:22:37ZCDS support team

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

cds-question@unistra.frsurveysyoung-stellar-objectsstellar-distancemillimeter-astronomyphotometrysubmillimeter-astronomyThe Herschel survey of the Galactic plane (Hi-GAL) provides a unique opportunity to study star formation over large areas of the sky and different environments in the Milky Way. We use the best-studied Hi-GAL fields to date, two 2{deg}x2{deg} tiles centered on (l,b)=(30{deg}, 0{deg}) and (l,b)=(59{deg},0{deg}), to study the star formation activity in these regions of the sky using a large sample of well-selected young stellar objects (YSOs). We used the science demonstration phase Hi-GAL fields, where a tremendous effort has been made to identify the newly formed stars and to derive their properties as accurately as possible, e.g. distance, bolometric luminosity, envelope mass, and stage of evolution. We estimated the star formation rate (SFR) for these fields using the number of candidate YSOs and their average time scale to reach the zero age main sequence, and compared it with the rate estimated using their integrated luminosity at 70um, combined with an extragalactic star formation indicator.2013A&A...549A.130Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/549/A130CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/526/A151 : Hi-Gal sources distance determination (Russeil+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/549/A130https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/549/A130http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/549/A130https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/549/A130https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/549/A130http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/549/A130GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/549/A130/yso (List of detected YSOs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/549/A130/yso?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/549/A130/yso?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/549/A130/yso?GETtext/xml+votable180.050000true280.638064-3.219410.0055555555555555565/3588 6/12975 12986 14341 14343 30257-30260 30262-30263 30265 30268-302693.2031150387835462e-22 1.000830682546041e-20https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/549/A130?format=asciiRadiodefaultJ/A+A/549/A130/ysoList of detected YSOsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameHi-GAL source name (GLLL.llll+B.bbbb)meta.id;meta.maincharGLONGalactic Longitudedegpos.galactic.lonGLATGalactic Latitudedegpos.galactic.latS24? Spitzer/MIPS 24 micron band fluxJyphot.flux.density;em.IR.15-30umfloatnullableS70Herschel/PACS 70 micron band fluxJyphot.flux.density;em.IR.30-60umfloatS160Herschel/PACS 160 micron band fluxJyphot.flux.density;em.mm.1500-3000GHzfloatS250Herschel/SPIRE 250 micron band fluxJyphot.flux.density;em.mm.750-1500GHzfloatS350Herschel/SPIRE 350 micron band fluxJyphot.flux.density;em.mm.750-1500GHzfloatS500? Herschel/SPIRE 500 micron band fluxJyphot.flux.density;em.mm.400-750GHzfloatnullabled[0/15] Kinematic distancekpcpos.distance;pos.heliocentricfloatSimbadSimbad column added by the CDSmeta.ref.urlchar_RA.icrsRight ascension (ICRS) (computed by VizieR, not part of the original data)degpos.eq.ranullableindexed_DE.icrsDeclination (ICRS) (computed by VizieR, not part of the original data)degpos.eq.decnullableindexed