An IRS survey of protoplanetary disk evolution in the Orion molecular-cloud complexes

Details An IRS survey of protoplanetary disk evolution in the Orion molecular-cloud complexes An IRS survey of protoplanetary disk evolution in the Orion molecular-cloud complexes

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop30706h&link_type=abstract

Spitzer Proposal ID #30706

Computer Science

Scientific paper

We propose to obtain IRS complete (5-40 micron) low-resolution spectra of a large sample of young stellar objects with protoplanetary disks in the Orion A and B molecular cloud complexes. The aim is to study the influence of the wide range of star-formation conditions in the Orion clouds on the structure, composition and evolution of protoplanetary disks, and on the conditions and occurrence of planet formation in these disks. This guaranteed-time observing program has a total of 100.9 hours, with 20 hours provided by IRAC PI Giovanni Fazio, 20 hours by MIPS PI George Rieke, and 60.9 hours by IRS PI Jim Houck.

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