GRÄFE, C.; WOLF, S.; SAUTER, J.; DUTREY, Anne; GUILLOTEAU, S.; SCHEGERER, A.; BEUTHER, H.; PADGETT, D. L.; STAPELFELDT, K. R.

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EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France, p.1031, 2011, EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France, p.1031, 2011, 2011, Nantes. 2011-10p. 1031

Résumé en anglais

We present first results of our self-consistent multiwavelength modeling of the Butterfly Star in Taurus. The continuum spectral energy distribution of the disk and envelope around this young stellar object as well as spatially resolved images in the range from 1 μm to 2.7mm are taken into account. In particular, a submillimeter observation at 894 μm and a new high angular resolution 1.3mm map obtained with the Submillimeter Array (SMA) and the Plateau de Bure Interferometer (PdBI), respectively, are considered for the first time.< Réduire

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