The Relationship of Atomic Gas and Aromatic Emission in SINGS Spiral Galaxies

Details The Relationship of Atomic Gas and Aromatic Emission in SINGS Spiral Galaxies The Relationship of Atomic Gas and Aromatic Emission in SINGS Spiral Galaxies

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...209.1503c&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #15.03; Bulletin of the American Astronomical Society, V

Astronomy and Astrophysics

Astronomy

Scientific paper

We present a comparison of emission from atomic gas and stochastically heated dust in two nearby, relatively face-on spirals, M51 and M74, using HI emission maps from THINGS and 8 micron dust emission from the SINGS Legacy project. This poster will describe initial results from an exploration of the extent to which Spitzer IRAC 8 micron emission traces the distribution of the interstellar medium and the star formation process in nearby spiral galaxies.

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