Characterizing the disk around the TW Hydrae Association brown dwarf 2MASSW J1207334-393254
arXiv:astro-ph/0702442 · doi:10.1086/516565
Abstract
We present detailed modeling of the disk around the TW Hydrae Association (TWA) brown dwarf 2MASSW J1207334-393254 (2M1207), using {\it Spitzer} observations from 3.6 to 24 $\micron$. The spectral energy distribution (SED) does not show a high amount of flaring. We have obtained a good fit using a flat disk of mass between and $M_{\sun}$, $\la10^{-11} M_{\sun}$/yr and a large inclination angle between 60$\degr$ and 70$\degr$. We have used three different grain models to fit the 10 $\micron$ Si emission feature, and have found the results to be consistent with ISM-like dust. In comparison with other TWA members, this suggests lesser dust processing for 2M1207 which could be explained by mechanisms such as aggregate fragmentation and/or turbulent mixing. We have found a good fit using an inner disk radius equal to the dust sublimation radius, which indicates the absence of an inner hole in the disk. This suggests the presence of a small K- excess, similar to the observed K-[3.6] excess.
19 pages, 4 figures, accepted in ApJ
References in corpus (7)
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- An Improbable Solution to the Underluminosity of 2M1207B: A Hot Protoplanet Collision Afterglow
- The Trigonometric Parallax of the Brown Dwarf Planetary System 2MASSW J1207334-393254
- New Brown Dwarf Disks in the TW Hydrae Association
- A Herschel Search For Cold Dust in Brown Dwarf Disks: First Results
- Surprisingly Weak Magnetism on Young Accreting Brown Dwarfs
- Metal Depletion and Warm H2 in the Brown Dwarf 2M1207 Accretion Disk
- The radial distribution of dust species in young brown dwarf disks
- Brown Dwarf Disks at Ages of 5-10 Myr
- Revised analysis of SPIRE observations for 2M1207
- JWST/MIRI observations of the young TWA 27 system: hydrocarbon disk chemistry, silicate clouds, evidence for a CPD