Computer Science
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40402f&link_type=abstract
Spitzer Proposal ID #40402
Computer Science
Scientific paper
We propose one IRAC map and two MIPS scan maps to extend (and complete) our map of W5. Previous MIPS observations (PID20300) just missed the deeply embedded star formation on the eastern--most edge of the HII region. One of the proposed MIPS observations will cover this region, matching our IRAC coverage. The second MIPS AOR will fill a narrow gap in the middle of our map at 70 microns, enabling us to complete our analysis of the dust emission in the bright rim surrounding W5. The current gap unfortunately passes along a ridge of 70 micron emission, where the two HII region bubble walls meet. The IRAC map covers the northeast corner of the bright rim, completing our map.
Allen Lori
Fazio Giovanni
Hora Joseph
Koenig Xavier
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