Spectral Mapping of NGC 1333

Details Spectral Mapping of NGC 1333 Spectral Mapping of NGC 1333

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop..116l&link_type=abstract

Spitzer Proposal ID #116

Computer Science

Scientific paper

We will carry out a spectral mapping of the central 17x25 arcmin of NGC 1333, a galactic molecular cloud rich in dense gas, very young stars, and outflows from low mass stars. Our primary goal is to map the spatial distribution of H2 rotational emission at 17 and 28 microns associated with the outflows. Additional goals are a study of the ice features associated with the embedded YSOs, and the identification of extended dust emission features. The results will be compared with existing millimeterwave CO maps and images of shocked gas from optical and near-IR wavelengths.

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