Investigation of Red Emission from Interstellar Dust Clouds

Details Investigation of Red Emission from Interstellar Dust Clouds Investigation of Red Emission from Interstellar Dust Clouds

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sptz.prop.3490k&link_type=abstract

Spitzer Proposal ID #3490

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Scientific paper

SDSS r, i and z maps of the Taurus dust clouds show that, unlike dust clouds seen in several other regions of sky, these clouds glow in the z band. We propose to make maps at all four IRAC bands of an approximately 1degreex1degree region of the Taurus clouds chosen to show a lot of structure in the red emission and a similar map of a region in the Orion dust clouds which does not show this emission. We hope, by combining and modeling these maps, to investigate the mechanism which produces the red glow and whether it is due to solid-state emission features from small grains.

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