J/MNRAS/450/4364ivo://CDS.VizieR/J/MNRAS/450/4364doi:10.26093/cds/vizier.74504364CDSNavarete F.Damineli A.Barbosa C.-L.Blum R.-D.2024-08-14T20:22:06Z2015-10-02T09:56:59ZCDS support team

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

cds-question@unistra.fryoung-stellar-objectsearly-type-starsinfrared-sourcesWe present the results from a survey, designed to investigate the accretion process of massive young stellar objects (MYSOs) through near infrared narrow band imaging using the H_2_ {nu}=1-0 S(1) transition filter. A sample of 353 Massive Young Stellar Object (MYSO) candidates was selected from the Red MSX Source survey using photometric criteria at longer wavelengths (infrared and submillimeter) and chosen with positions throughout the Galactic Plane. Our survey was carried out at the SOAR Telescope in Chile and CFHT in Hawaii covering both hemispheres.2015MNRAS.450.4364Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/450/4364CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/474/891 : 13CO observations of YSOs in South Gal. plane (Urquhart+ 2007)J/A+A/487/253 : The RMS survey: ^13^CO observations of YSOs (Urquhart+ 2008)J/A+A/525/A149 : Red MSX Survey: bolometric fluxes of YSOs (Mottram+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/450/4364https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/450/4364http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/450/4364https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/450/4364https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/450/4364http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/450/4364GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/450/4364/sources (Log of observations (table 1) and general classification of the sources (table 2))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/450/4364/sources?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/450/4364/sources?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/450/4364/sources?GETtext/xml+votable180.050000true275.2303333-14.25855560.005555555555555556Cone search capability for table J/MNRAS/450/4364/table4 (Properties of the potential stellar clusters identified on each field)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/450/4364/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/450/4364/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/450/4364/table4?GETtext/xml+votable180.050000true279.19583-7.594170.0055555555555555565/7383 6/1344 1930 3157 3175 3184 3195 3198 3271 3290 3302 3311 3320 3630 3649 3715 3729 3747 14063 14241 14280 14282 14304 14307 14311 14315 14317 14365 14622 14664 14666 14670 14682-14683 14689-14691 14696-14697 14704 14706 15370 15414 15428 15430 15434 15448-15449 15452 15468 15476 15624 15649 15681 15696 20831 21504 21510 21639 21643 21645 21670 22040 22065 22070 22122 22124 22173 22243 23636-23637 23639 23666 23764 23766 23773 23968-23969 23982 24325 24554 29461 29463 29504 29507 29509 29511 29517 29522 29529 30218-30219 30222 30241 30244-30245 30257-30258 30262-30263 30268-30269 30314-30315 30319 30405 30416-30417 30419 30421 30592 30594 30598 30600 30605-30607 30618-30619 30622 30716 37333 37343 37362 37366 37369 37372 37732 37831 37848-37850 37855 37860 37872 37884 37886-37887 37893-37896 37902 37922 37924 37928 37934 38016 38019 39240 39246 39248 39258 39270 39273 39276 39282 39375 39404 39803 41595 41654-41655 41658 41671 41673 41675-41678 41681-41683 41685 41698 41702 41740 41758-41759 41763 41767 41770 41772 41777-41778 41780 41782 41804-41805 41811 41813-41814 41817 41820 41824 42159 42168-42170 42172-42173 42207 42213-42216 42224 42227-42230 42233 42376 42379 42383 42392 42397-42398 42434 42441 42444 42496-42498 42512 43014-43015 43019 43021 43026https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/450/4364?format=asciiInfrareddefaultJ/MNRAS/450/4364/sourcesLog of observations (table 1) and general classification of the sources (table 2)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPropindicates properties in tables 3 and/or 4meta.ref.urlcharIDSource sequential numbermeta.idintprimaryMSXMSX name (GLLL.llll+BB.bbbb)meta.id;meta.maincharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainDistKinematic distance of the source (1)kpcpos.distance;pos.heliocentricfloatlogLumBolometric luminosity of the source (2)log(solLum)phys.luminosityfloatTelTelescope usedinstr.setupcharSemSemester of the Observationtime.epochcharCnt[Y/N] Extended continuum emissionmeta.codecharClu[Y/N] Association with stellar cluster candidatemeta.codecharH2pPrimary H_2_ classificationmeta.code.classcharH2sSecondary H_2_ classificationmeta.code.classcharH2cH_2_ componentsmeta.code.multipcharJ/MNRAS/450/4364/table3Properties of the H_2_ structures identified on each fieldrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDSource sequential numbermeta.idintComptype of the structure (H_2_ emission or cluster)meta.code.multipcharlproj? Projected length of first component (1)pcpos.distancefloatnullablelproj2? Projected length of second component (1)pcpos.distancefloatnullablelproj3? Projected length of third component (1)pcpos.distancefloatnullablelproj4? Projected length of fourth component (1)pcpos.distancefloatnullablePA? Position angle of first component (2)degpos.posAngintnullablePAu? Upper value of position angle of first component when interval (2)degpos.posAng;stat.maxintnullablePA2? Position angle of second component (2)degpos.posAngintnullablePA3? Position angle of third component (2)degpos.posAngintnullablePA4? Position angle of fourth component (2)degpos.posAngintnullablePA5? Position angle of fifth component (2)degpos.posAngintnullablePA6? Position angle of sixth component (2)degpos.posAngintnullableRst? Aspect ratio of first component for polar structuressrc.morph.paramfloatnullableRst2? Aspect ratio of second component for polar structuressrc.morph.paramfloatnullableRst3? Aspect ratio of third component for polar structuressrc.morph.paramfloatnullableRst4? Aspect ratio of fourth component for polar structuressrc.morph.paramintnullableJ/MNRAS/450/4364/table4Properties of the potential stellar clusters identified on each fieldrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDSource sequential numbermeta.idintRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainDistKinematic distance of the MSX source (1)kpcpos.distance;pos.heliocentricfloatlprojProjected angular diameter of the clusterpcpos.distancefloatDiamAngular diameter of the clusterarcsecphys.angSizeint