Centers of activity in dust clouds

Details Centers of activity in dust clouds Centers of activity in dust clouds

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.128..217c&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

Infrared Astronomy, Infrared Stars, Interstellar Matter, Molecular Clouds, Star Formation, Emission Spectra, Galaxies, H Ii Regions, Infrared Spectra, Stellar Envelopes, Submillimeter Waves

Scientific paper

Recent submm observations of dust emission from star-forming regions are presented and combined with NIR and IRAS data. The spectra cover the range 0.3 to 1300 microns and originate from ZAMS stars, compact H II regions, low-luminosity objects in dark clouds, and external galaxies. The dust emission spectra are interpreted in terms of density and temperature distributions around central heating sources. In addition, general properties like IR luminosity, optical depth, wavelength dependence of dust opacity, and, in the case of galaxies, star formation efficiency are discussed.

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