J/A+A/569/A11ivo://CDS.VizieR/J/A+A/569/A11doi:10.26093/cds/vizier.35690011CDSSanchez-Monge A.Beltran M.T.Cesaroni R.Etoka S.Galli D.,Kumar M.S.N.Moscadelli L.Stanke T.van der Tak F.F.S.Vig S.,Walmsley C.M.Wang K.-S.Zinnecker H.Elia D.Molinari S.Schisano E2015-02-08T13:01:46Z2014-09-09T10:55:33ZCDS support team

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

cds-question@unistra.fryoung-stellar-objectsmillimeter-astronomyphotometrysubmillimeter-astronomyThe formation process of high-mass stars (with masses >8M_{sun}_) is still poorly understood, and represents a challenge from both the theoretical and observational points of view. The advent of the Atacama Large Millimeter Array (ALMA) is expected to provide observational evidence to better constrain the theoretical scenarios. The present study aims at characterizing the high-mass star forming region G35.20-0.74N, which is found associated with at least one massive outflow and contains multiple dense cores, one of them recently found associated with a Keplerian rotating disk. We used the radio-interferometer ALMA to observe the G35.20-0.74N region in the submillimeter continuum and line emission at 350GHz. The observed frequency range covers tracers of dense gas (e.g., H^13^CO^+^, C^17^O), molecular outflows (e.g., SiO), and hot cores (e.g., CH_3_CN, CH_3_OH). These observations were complemented with infrared and centimeter data.2014A&A...569A..11Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/569/A11CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/569/A11https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/569/A11http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/569/A11https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/569/A11https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/569/A11http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/569/A11GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/569/A11/maps (List of FIT files)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/569/A11/maps?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/569/A11/maps?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/569/A11/maps?GETtext/xml+votable180.050000true284.55431.676660.0055555555555555566/30319https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/569/A11?format=asciiRadiodefaultJ/A+A/569/A11/mapsList of FIT filesNx[512] Number of pixels along X-axismeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right Ascension of center (J2000)degpos.eq.ra;meta.mainDEJ2000Declination of center (J2000)degpos.eq.dec;meta.mainScale[0.08] Scale of the imagearcsec/pixinstr.scalefloatNy[512] Number of pixels along Y-axismeta.numberintNz[30/1000]? Number of slices for datacubesmeta.numberintnullableRVmin[-300/0]? Lower value of radial velocity interval for data cubeskm/sphys.velocfloatnullableRVmax[58/400]? Upper value of radial velocity interval for data cubeskm/sphys.velocfloatnullabledRV[0.6/2]? Velocity resolutionkm/sspect.dopplerVelocfloatnullableFreq[335/351]? Frequency of line observedGHzem.freq;spect.linefloatnullablesize[1/1001] Size of FITS fileMibytephys.size;meta.fitsfloatfitsDownload the FITS filemeta.ref.urlcharFileNameName of FITS file in subdirectory fitsmeta.id;meta.fitscharTitleTitle of the filemeta.title;meta.file