BROWN DWARF DISKS AT AGES OF 5-10 Myr

Basmah Riaz, Nicolas Lodieu, John E. Gizis

    Research output: Contribution to journalArticlepeer-review

    19 Citations (Scopus)

    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 languageEnglish
    Pages (from-to)1173-1182
    Number of pages10
    JournalThe Astrophysical Journal
    Volume705
    Issue number2
    DOIs
    Publication statusPublished - 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

    Fingerprint

    Dive into the research topics of 'BROWN DWARF DISKS AT AGES OF 5-10 Myr'. Together they form a unique fingerprint.

    Cite this