The circumstellar disk of HH30: Searching for signs of disk evolution with multi-wavelength modeling
Langue
en
Communication dans un congrès
Ce document a été publié dans
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France, p.409, 2011, EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France, p.409, 2011, 2011, Nantes. 2011-10p. 409
Résumé en anglais
We conducted a parameter study based on simulated annealing to construct a self-consistent model of HH30's circumstellar disk using all available observations in the wavelength domain 1μm. . . 3mm. Recently made high-resolution ...Lire la suite >
We conducted a parameter study based on simulated annealing to construct a self-consistent model of HH30's circumstellar disk using all available observations in the wavelength domain 1μm. . . 3mm. Recently made high-resolution observations of continuum visibilities at = 1.3mm with the Plateau de Bure Interferometer [1] and the spectral energy distribution (SED) in the mid infrared with IRS on the Spitzer Space Telescope (SST) [2] significantly increased constraints on our modeling attempt. We present models of the edge-on disk featuring an inner depletion zone with 100AU diameter explaining subsets of the available data and conclude the presence of dust growth and settling.< Réduire
Origine
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