Protoplanetary disk evolution in the Orion, Serpens and Perseus clouds

Details Protoplanetary disk evolution in the Orion, Serpens and Perseus clouds Protoplanetary disk evolution in the Orion, Serpens and Perseus clouds

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40525h&link_type=abstract

Spitzer Proposal ID #40525

Computer Science

Scientific paper

We propose to obtain complete IRS low-resolution spectra (5-40 micron) of a large sample of young stellar objects with protoplanetary disks and envelopes in molecular cloud complexes in Orion B (the NGC 2024 and 2068 clusters), the NGC 1333 cluster in Perseus, and the main young cluster in Serpens. The aim is to study the influence of the wide range of well-characterized star-formation conditions represented by these clouds on the structure, composition and evolution of protoplanetary disks and protostellar envelopes, and on the conditions and occurrence of planet formation in these disks. This guaranteed-time observing program has a total of 88.4 hours, with 15 hours provided by IRAC PI Giovanni Fazio, 15 hours by MIPS PI George Rieke, and 53.4 hours by IRS PI Jim Houck.

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