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

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

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1031g&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1031

Physics

Scientific paper

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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