Balmer-line equivalent widths in main sequence B-F stars, and comparison with model atmospheres

Details Balmer-line equivalent widths in main sequence B-F stars, and comparison with model atmospheres Balmer-line equivalent widths in main sequence B-F stars, and comparison with model atmospheres

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981sva....25...45d&link_type=abstract

(Astronomicheskii Zhurnal, vol. 58, Jan.-Feb. 1981, p. 80-90.) Soviet Astronomy, vol. 25, Jan.-Feb. 1981, p. 45-49. Translation

Astronomy and Astrophysics

Astronomy

2

A Stars, Atmospheric Models, B Stars, Balmer Series, F Stars, Main Sequence Stars, Spectral Line Width, Stellar Atmospheres, H Lines, Stellar Spectra, Stellar Spectrophotometry

Scientific paper

Equivalent widths of the Balmer H-alpha, H-beta, and H-gamma lines were measured for 175 main-sequence B-F stars and compared with curves calculated from various model stellar atmospheres. When averaged over each spectral subtype, the equivalent widths are well represented by the standard models; this confirms the previous finding of Glushneva and Doroshenko (1980) that the models are fully consistent with the observations.

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