Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sva....26..316g&link_type=abstract
(Astronomicheskii Zhurnal, vol. 59, May-June 1982, p. 523-535.) Soviet Astronomy, vol. 26, May-June 1982, p. 316-323. Translati
Astronomy and Astrophysics
Astronomy
A Stars, B Stars, Balmer Series, Stellar Spectra, Angular Velocity, Continuous Spectra, Spectral Energy Distribution, Spectral Line Width, Stellar Models, Stellar Rotation
Scientific paper
The characteristics of the continuous spectrum and the equivalent widths of H-alpha, H-beta, and H-gamma, Balmer lines of rapidly rotating stars are investigated. A comparison is made with the analogous characteristics for stars with low rotation rates and with theoretical values calculated from models of rotating stars. The limits of variation of the angle of orientation of the rotation axis are determined for several stars on the basis of a comparison with models.
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