Intensity and width of the excited hydrogen radiolines in Orion nebulae

Details Intensity and width of the excited hydrogen radiolines in Orion nebulae Intensity and width of the excited hydrogen radiolines in Orion nebulae

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51.1237g&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, Nov.-Dec. 1974, p. 1237-1244. In Russian.

Astronomy and Astrophysics

Astronomy

5

H Lines, Nebulae, Radio Spectra, Spectral Line Width, Astronomical Models, Hydrogen Clouds, Line Spectra, Radio Astronomy, Stark Effect

Scientific paper

For a model of Orion nebulae consisting of condensations with Ne approximately equal to 10 to the fourth power in the nucleus and rarefied extended shell the intensity and width of the excited hydrogen radiolines are calculated. The possibility has been shown to explain for this model the experimental data which exist, in particular, in the absence of the expected Stark broadening.

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