Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196..723j&link_type=abstract
Astrophysical Journal, vol. 196, Mar. 15, 1975, pt. 1, p. 723-731.
Astronomy and Astrophysics
Astronomy
15
Emission Spectra, H Alpha Line, Interstellar Gas, Radiative Recombination, Radio Spectra, Electronic Spectra, Galactic Radiation, Galactic Structure, H I Regions, H Ii Regions, Ionized Gases, Line Spectra, Milky Way Galaxy, Position (Location), Radio Sources (Astronomy), Thermal Radiation
Scientific paper
In the discussion of the results of the investigation attention is given to emission nonuniformity, emission location, the electron temperature for the line-emitting region, the emission measure, the nature of the emission, small H II regions, elongated H II complexes, large and hot H I regions, small and cold clouds, and mixed emitting regions. Profile patterns indicate that the H 110-alpha recombination-line emission observed for the range from 24 deg to 33 deg originates in small-scale structures along the line of sight.
Jackson Paul D.
Kerr Frank J.
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