H66-alpha radio recombination line observations of southern H II regions

Details H66-alpha radio recombination line observations of southern H II regions H66-alpha radio recombination line observations of southern H II regions

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193..737a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Dec. 1980, p. 737-743. Research supported by the Financiadora Naci

Astronomy and Astrophysics

Astronomy

1

H Alpha Line, H Ii Regions, Nebulae, Radio Spectra, A Stars, Abundance, Electron Density Profiles, Helium

Scientific paper

The H66-alpha recombination line has been observed in Orion A and in
four prominent southern H II regions: RCW 38, Car I, RCW 57 and Norma
III. The physical parameters (1) line-to-continuum temperature ratio,
(2) line halfwidth, and (3) LTE electron temperature, are given.

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