Submm/far-infrared observations of cold and warm dust clouds

Details Submm/far-infrared observations of cold and warm dust clouds Submm/far-infrared observations of cold and warm dust clouds

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.128..111m&link_type=abstract

(Universitaets-Sternwarte Jena, Jena Workshop on the Role of Dust in Dense Regions of Interstellar Matter, Georgenthal, East Ger

Astronomy and Astrophysics

Astronomy

1

Cosmic Dust, Infrared Astronomy, Interstellar Matter, Molecular Clouds, Submillimeter Waves, B Stars, Emission Spectra, Infrared Spectra, O Stars, Spiral Galaxies

Scientific paper

Sub-mm/FIR emission from the Galactic disk and center regions is used to illustrate the dust emission from complex regions in interstellar space that can be discerned in cold dust heated by the general interstellar radiation field and emission from OB star-heated warm dust. Only O and early B stars are sufficiently luminous and numerous to account for an observed warm dust luminosity of nearly 10 to the 10th solar luminosities.

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