Protostars and Planets VI, Heidelberg, July 15-20, 2013
Poster 2B012
Correlations between the stellar and disc properties of Taurus PMS stars in the GASPS sample
Alonso-Martínez, Miguel (Depto. de Física Teórica, Fac Ciencias, UAM Campus Cantoblanco, 28049 Madrid, Spain)
Riviere-Marichalar, Pablo (Kapteyn Astronomical Institute P.O. Box 800 9700 AV Groningen, The Netherlands)
Pascual, Natalia (Depto. de Física Teórica, Fac Ciencias, UAM Campus Cantoblanco, 28049 Madrid, Spain)
Montesinos, Benjamín (Centro de Astrobiología - Depto. Astrofísica (CSIC-INTA), POB 78, 28691 Villanueva de la Cañada, Spain)
Howard, Christian D. (SOFIA - USRA, NASA Ames Research Center, USA)
Sandell, Göran (SOFIA - USRA, NASA Ames Research Center, USA)
Meeus, Gwendolyn (Depto. de Física Teórica, Fac Ciencias, UAM Campus Cantoblanco, 28049 Madrid, Spain)
Eiroa, Carlos (Depto. de Física Teórica, Fac Ciencias, UAM Campus Cantoblanco, 28049 Madrid, Spain)
Dent, Bill (ALMA, Avda Apoquindo 3846, Piso 19, Edificio Alsacia, Las Condes, Santiago, Chile )
Abstract:
The Herschel Open Time Key Programme GASPS (P.I. B. Dent) has observed a large number of pre-main sequence TTauri stars in Taurus with PACS (photometry and spectroscopy). In addition, we have also carried out new ground-based optical and near-IR observations (photometry and spectroscopy) of most of the Taurus GASPS sample. In this poster, we present some preliminary results on correlations between the stellar and disc properties of this young stellar sample.
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