Intensity and width of radio lines of excited hydrogen in the Orion nebula

Details Intensity and width of radio lines of excited hydrogen in the Orion nebula Intensity and width of radio lines of excited hydrogen in the Orion nebula

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....18..737g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 51, Nov.-Dec. 1974, p. 1237-1244.) Soviet Astronomy, vol. 18, May-June 1975, p. 737-741. Transl

Astronomy and Astrophysics

Astronomy

1

H Lines, Nebulae, Radio Spectra, Spectral Line Width, Astronomical Models, Hydrogen Clouds, Line Spectra, Radiant Flux Density, 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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