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25 April 2024
 
  » arxiv » 0803.2051

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Structural and compositional properties of brown dwarf disks: the case of 2MASS J04442713+2512164
H. Bouy ; N. Huelamo ; C. Pinte ; J. Olofsson ; D. Barrado y Navascues ; E. L. Martin ; E. Pantin ; J.-L. Monin ; G. Basri ; J.-C. Augereau ; F. Menard ; G. Duvert ; G. Duchene ; F. Marchis ; A. Bayo ; S. Bottinelli ; B. Lefort ; S. Guieu ;
Date 13 Mar 2008
AbstractIn order to improve our understanding of substellar formation, we have performed a compositional and structural study of a brown dwarf disk.
We present the result of photometric, spectroscopic and imaging observations of 2MASS J04442713+2512164, a young brown dwarf (M7.25) member of the Taurus association. Our dataset, combined with results from the literature, provides a complete coverage of the spectral energy distribution from the optical to the millimeter including the first photometric measurement of a brown dwarf disk at 3.7mm, and allows us to perform a detailed analysis of the disk properties.
The target was known to have a disk. High resolution optical spectroscopy shows that it is intensely accreting, and powers a jet and an outflow. The disk structure is similar to that observed for more massive TTauri stars. Spectral decomposition models of Spitzer/IRS spectra suggest that the mid-infrared emission from the optically thin disk layers is dominated by grains with intermediate sizes (1.5micron). Crystalline silicates are significantly more abondant in the outer part and/or deeper layers of the disk, implying very efficient mixing and/or additional annealing processes. Sub-millimeter and millimeter data indicate that most of the disk mass is in large grains (>1mm)
Source arXiv, 0803.2051
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