Multi-wavelength modeling of the circumstellar disk of the Butterfly Star in Taurus

C. Gräfe S. Wolf J. Sauter Anne Dutrey 1 S. Guilloteau 1 A. Schegerer H. Beuther 2 D. L. Padgett K. R. Stapelfeldt
1 aMOR 2011
L3AB - Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux, OASU - Observatoire aquitain des sciences de l'univers, LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac], Université Sciences et Technologies - Bordeaux 1
Abstract : 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.
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https://hal.archives-ouvertes.fr/hal-00665195
Contributeur : Marie-Paule Pomies <>
Soumis le : mercredi 1 février 2012 - 13:37:20
Dernière modification le : mercredi 29 novembre 2017 - 15:00:38

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C. Gräfe, S. Wolf, J. Sauter, Anne Dutrey, S. Guilloteau, et al.. Multi-wavelength modeling of the circumstellar disk of the Butterfly Star in Taurus. EPSC-DPS Joint Meeting 2011, 2011, Nantes, France. pp.1031, 2011. 〈hal-00665195〉

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