Disk Evolution in the Planet Formation Epoch

Details Disk Evolution in the Planet Formation Epoch Disk Evolution in the Planet Formation Epoch

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...37f&link_type=abstract

Spitzer Proposal ID #37

Computer Science

Scientific paper

The goal of this program is to trace the evolution of circumstellar disks around young stars through the likely epoch of planet formation at around 5-10 Myr. Disk spectral energy distributions will be used to determine the times of disk clearing as a function of radius, age, and stellar mass. IRAC and MIPS will be used to study circumstellar dust emission, with special emphasis on objects in the age range 3-10 Myr which are vastly underrepresented in current samples. Studies of nearby regions in Taurus and Chamaeleon I are included for comparison, along with objects in the nearby eta Cha and TW Hya associations.

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