Deep IRAC Imaging of Brown Dwarfs in Star Forming Clusters

Details Deep IRAC Imaging of Brown Dwarfs in Star Forming Clusters Deep IRAC Imaging of Brown Dwarfs in Star Forming Clusters

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...36f&link_type=abstract

Spitzer Proposal ID #36

Physics

Scientific paper

Deep IRAC imaging will be used to measure 1) the substellar IMF (>0.5-1 M_jup) and 2) the 1-8um SEDs of young brown dwarf/disk systems (>1-2 M_jup) within the three nearby star forming clusters (0.5-2 Myr) of IC 348 (300 pc), Rho Oph (150 pc), and Cha I (150 pc). The maps of these clusters will have dimensions of 15'x15', 10'x10', and 15'x15' and total exposure times per pointing of 3000, 3000, and 2000 s.

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