Abstract
We present Spitzer/IRAC and MIPS 24 mu m observations for 28 brown dwarfs in the Upper Scorpius (UppSco) region. We find a disk fraction of 10.7%-(+ 8.7%)(3.3%) . One object shows a small excess at 24 mu m but none at shorter wavelengths, and may be a candidate transition disk. Three objects show emission in the 10 mu m silicate feature and we present compositional fits for these sources. Flat structures are observed for all disk sources in UppSco. Also presented are the MIPS/70 mu m observations for the TW Hydrae Association brown dwarf 2MASS J1139511-315921. We discuss the structure and chemistry of brown dwarf disks at ages of similar to 5-10 Myr, and consider the possible effects of the brown dwarf densities in these clusters on the disk lifetimes.
Original language | English |
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Pages (from-to) | 1173-1182 |
Number of pages | 10 |
Journal | The Astrophysical Journal |
Volume | 705 |
Issue number | 2 |
DOIs | |
Publication status | Published - 10 Nov 2009 |
Keywords
- circumstellar matter
- open clusters and associations: individual (Taurus, Upper Scorpius)
- stars: low-mass, brown dwarfs
- SCORPIUS OB ASSOCIATION
- TW-HYDRAE-ASSOCIATION
- LOW-MASS STARS
- MAIN-SEQUENCE STARS
- LARGE-AREA SEARCH
- TAURI STARS
- FORMING REGION
- GRAIN-GROWTH
- PROTOPLANETARY DISKS
- SPITZER OBSERVATIONS