Dust Mass and Spatial Structure in the ISM

Details Dust Mass and Spatial Structure in the ISM Dust Mass and Spatial Structure in the ISM

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21522704g&link_type=abstract

American Astronomical Society, AAS Meeting #215, #227.04; Bulletin of the American Astronomical Society, Vol. 42, p.545

Astronomy and Astrophysics

Astronomy

Scientific paper

The SAGE-LMC and SAGE-SMC Spitzer Legacy programs have provided full IRAC/MIPS images of both Magellanic Clouds. These images have been used to map the spatial distribution of interstellar dust in these two nearby galaxies and study how this dust correlates with atomic (traced by HI) and molecular (traced by CO). Studies of these correlations, the variations between the Clouds, and what they reveal about the ISM structure will be summarized. Preliminary results on dust masses from Herschel observations of the LMC taken as part of the HERITAGE Key Project may also be presented.

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