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hal.structure.identifierHerschel Science Center [Madrid]
dc.contributor.authorRIBAS, Á.
dc.contributor.authorESPAILLAT, C. C.
dc.contributor.authorMACIAS, E.
hal.structure.identifierM2A 2018
dc.contributor.authorBOUY, H.
dc.contributor.authorANDREWS, S.
dc.contributor.authorCALVET, N.
hal.structure.identifierUniversity of Lethbridge
dc.contributor.authorNAYLOR, D. A.
hal.structure.identifierDepartamento de Astrofisica [Madrid]
dc.contributor.authorRIVIERE-MARICHALAR, P.
dc.contributor.authorVAN DER WIEL, M. H. D.
hal.structure.identifierCentre for Astronomy
dc.contributor.authorWILNER, D.
dc.date.issued2018
dc.descriptionVizieR On-line Data Catalog: J/ApJ/849/63. Originally published in: 2017ApJ...849...63R
dc.description.abstractEnWe considered the 161 Taurus objects studied by Furlan+ (2011ApJS..195....3F), 134 objects in Ophiuchus in McClure+ (2010ApJS..188...75M), and the 84 objects in Chamaeleon I analyzed in Manoj+ (2011ApJS..193...11M). These studies presented and analyzed Spitzer/IRS spectra of these disks, and performed a detailed study of the properties of their inner regions. After analysis (see section 2 for the details), the sample size has been reduced to 284 YSOs: 154 in Taurus, 70 in Ophiuchus, and 60 in Chamaeleon I. We processed a number of scan and cross scan maps available in the Herschel Science Archive to achieve a satisfactory coverage of the three regions considered in this study. All of them were obtained by the Herschel Gould Belt Survey (P.I.: Philippe Andre), except for one set of observations in Ophiuchus (P.I.: Peter Abraham). See tables 11-13. (9 data files).
dc.language.isoen
dc.subject.enStar Forming Region
dc.subject.enEnergy distributions
dc.subject.enPhotometry: infrared
dc.subject.enPhotometry: millimetric/submm
dc.subject.enYSOs
dc.title.enVizieR Online Data Catalog: FIR-mm data of YSOs in star-forming regions (Ribas+, 2017)
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
hal.identifierhal-01982288
hal.version1
hal.popularnon
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01982288v1
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