RIBAS, Á.; ESPAILLAT, C. C.; MACIAS, E.; BOUY, H.; ANDREWS, S.; CALVET, N.; NAYLOR, D. A.; RIVIERE-MARICHALAR, P.; VAN DER WIEL, M. H. D.; WILNER, D.

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RIBAS, Á.
Herschel Science Center [Madrid]

ESPAILLAT, C. C.

MACIAS, E.

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Ce document a été publié dans

2018

Résumé en anglais

We 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).< Réduire

Mots clés en anglais

Star Forming Region

Energy distributions

Photometry: infrared

Photometry: millimetric/submm

YSOs

Origine

Importé de hal

Unités de recherche

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804