The infrared appearance of dusty H II regions

Details The infrared appearance of dusty H II regions The infrared appearance of dusty H II regions

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45..301k&link_type=abstract

(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital

Astronomy and Astrophysics

Astronomy

Cosmic Dust, H Ii Regions, Infrared Astronomy, Interstellar Extinction, Nebulae, Radio Astronomy, Black Body Radiation, Brightness Temperature, Lyman Spectra, O Stars, Radiative Transfer, Stellar Temperature

Scientific paper

Theoretical models of dusty H II regions are examined from the viewpoint of accounting for certain observational IR and radio data. The observational features considered include the position of the IR maximum, the color temperatures on either side of the peak, accurate profiles of brightness temperatures across the nebula at different frequencies, and the ratio of the He II to the H II zones.

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