Cold Dust and Very Cold Excess Emission in the Galaxy

Details Cold Dust and Very Cold Excess Emission in the Galaxy Cold Dust and Very Cold Excess Emission in the Galaxy

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.281..243b&link_type=abstract

Astrophysics and Space Science, v. 281, Issue 1, p. 243-246 (2002).

Astronomy and Astrophysics

Astrophysics

2

Dust, The Galaxy, Infrared

Scientific paper

We provide insight in the origin of the far-IR to mm emission from galaxies by presenting a decomposition of the Galaxy emission where we separate the contributions from dust in the atomic gas and dust associated with quiescent molecular gas as a function of Galacto-centric distance. This decomposition leaves a puzzling very cold emission excess with a brightness independent of Galactic longitude that might be pointing at interstellar matter in the outer Galaxy not traced by H I nor CO emission.

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