Spectral energy distribution of main-sequence B-F stars, and comparisons with theory

Details Spectral energy distribution of main-sequence B-F stars, and comparisons with theory Spectral energy distribution of main-sequence B-F stars, and comparisons with theory

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980azh....57..731g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 57, July-Aug. 1980, p. 731-737.) Soviet Astronomy, vol. 24, July-Aug. 1980, p. 421-424. Transla

Astronomy and Astrophysics

Astronomy

B Stars, F Stars, Main Sequence Stars, Spectral Energy Distribution, Stellar Atmospheres, Stellar Spectra, Stellar Spectrophotometry, Atmospheric Models, Balmer Series, Electrophotometers, Stellar Temperature

Scientific paper

Four spectrophotometric gradients in the 3200-7600 A wavelength range, together with the Balmer discontinuity, are evaluated on the basis of photoelectric measurements of the spectral energy distribution of 152 main-sequence B1-G0 stars. The curves for these quantities as functions of effective temperature conform closely to values calculated from several different model atmospheres.

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