Some Properties of the Spectral Emissivity of the Dust in the Submillimeter/Millimeter

Details Some Properties of the Spectral Emissivity of the Dust in the Submillimeter/Millimeter Some Properties of the Spectral Emissivity of the Dust in the Submillimeter/Millimeter

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..414..372d&link_type=abstract

Cosmic Dust - Near and Far ASP Conference Series, Vol. 414, proceedings of a conference held 8-12 September 2008 in Heidelberg,

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In this article, we describe the research on dust spectra which has been performed with the PRONAOS balloon-borne experiment, as well as other insights on dust spectral properties. Results show a clear dependence of the spectral emissivity on the temperature of the medium. The temperature itself varies a lot in both star-forming and quiet environments, so that taking into account temperature and spectral emissivity variations into dust models and templates for CMB data analysis is necessary.

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