IRAC Imaging of NGC4013

Details IRAC Imaging of NGC4013 IRAC Imaging of NGC4013

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop..215f&link_type=abstract

Spitzer Proposal ID #215

Physics

Scientific paper

The proposed IRAC observations will characterize the disk properties of NGC 4013 in the infrared with unprecedented detail -- disk scale lengths and scale heights in all four IRAC bands, the location and strength of star formation within the disk, and the putative warp. The IRAC data will be particularly sensitive to the expected strong PAH emission. The resulting mosaiced image will make a striking contrast with existing visible wavelength images (e.g., HST NICMOS and WFPC2) that show a strong band of dust attenuation along the center of the disk; IRAC will reveal the underlying stellar emission.

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