An IRAC Survey of the L1630 and L1641 (Orion) Molecular Clouds

Details An IRAC Survey of the L1630 and L1641 (Orion) Molecular Clouds An IRAC Survey of the L1630 and L1641 (Orion) Molecular Clouds

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...43f&link_type=abstract

Spitzer Proposal ID #43

Computer Science

Scientific paper

We will conduct a survey of the Orion A (L1641) and Orion B (l1630) Molecular Clouds in all four IRAC bands. From this survey we can achieve the following: 1.) probe the spatial distribution of young stars in the Orion clouds, comparing the number of clustered and isolated stars, 2.) study the evolution of circumstellar disks and envelopes during the first few millions years of pre--main sequence evolution, and 3.) measure the Orion cloud IMF down to 10-20 Mjupiter.

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