Nature of the Millimeter Excess Emission in the Magellanic Clouds

Details Nature of the Millimeter Excess Emission in the Magellanic Clouds Nature of the Millimeter Excess Emission in the Magellanic Clouds

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21724318p&link_type=abstract

American Astronomical Society, AAS Meeting #217, #243.18; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Using Planck maps combined with IRAS data, we construct dust apparent
temperature and optical depth in the Small and Large Magellanic Clouds.
The spatial distribution of the dust optical depth is used to constrain
the nature of the millimeter excess in these low metallicity galaxies.

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