Dust Properties Throughout the Milky Way

Details Dust Properties Throughout the Milky Way Dust Properties Throughout the Milky Way

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21724323p&link_type=abstract

American Astronomical Society, AAS Meeting #217, #243.23; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Planck observes the entire sky from 30 to 857 GHz. The observed foreground emission contains contributions from different phases of the interstellar medium that vary as a function of Galactic radius. We show how the Planck galactic emission separates into different gaseous components (atomic, molecular, and ionised) as well as into a number of Galactocentric rings. This technique provides the necessary information to study dust properties (emissivity, temperature, dust to gas ratio...) throughout the Milky Way.

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