Disk structure and planet formation around young low-mass stars and brown dwarfs

Details Disk structure and planet formation around young low-mass stars and brown dwarfs Disk structure and planet formation around young low-mass stars and brown dwarfs

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop30540h&link_type=abstract

Spitzer Proposal ID #30540

Computer Science

Scientific paper

We propose to obtain IRS complete (5-40 micron) low-resolution spectra of a sample of 41 young low-mass stars and brown dwarfs, to study the characteristics of their disks and to search for evidence of ongoing planet formation. We also propose to use IRAC to observe an additional 43 newly-identified brown dwarfs in Taurus and Chamaeleon, for future IRS spectroscopic followup. This guaranteed-time observing program has a total of 50.1 hours, with 14 hours provided by IRAC PI Giovanni Fazio, and 36.1 hours by IRS PI Jim Houck.

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