A MIPS Survey of the Orion L1641 and L1630 Molecular Clouds

Details A MIPS Survey of the Orion L1641 and L1630 Molecular Clouds A MIPS Survey of the Orion L1641 and L1630 Molecular Clouds

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop...47f&link_type=abstract

Spitzer Proposal ID #47

Physics

Scientific paper

We plan MIPS observations of the Orion L1630 and L1641 clouds. In conjunction with IRAC imaging, we will obtain the spectral energy distribution of the entire Orion young star population from 3.6-70 um. These data will be used to study the evolution of circumstellar disks and envelopes during the first few million years of pre-main sequence evolution and survey the clouds for embedded protostars.

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