Multi-wavelength modeling of the circumstellar disk of the Butterfly Star in Taurus
Language
en
Communication dans un congrès
This item was published in
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
English 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 ...Read more >
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.Read less <
Origin
Hal imported