Spectrophotometry B, A, and F stars. III

Details Spectrophotometry B, A, and F stars. III Spectrophotometry B, A, and F stars. III

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...266..732a&link_type=abstract

Astrophysical Journal, Part 1, vol. 266, Mar. 15, 1983, p. 732-738. Research supported by the Citadel Development Foundation an

Astronomy and Astrophysics

Astrophysics

25

A Stars, B Stars, Early Stars, F Stars, Stellar Spectrophotometry, Stellar Temperature, Solar Atmosphere, Spectral Energy Distribution, Stellar Atmospheres, Stellar Spectra, Ultraviolet Photometry

Scientific paper

Optical region energy distributions of 13 bright normal B, A, and F stars consistent with the Hayes-Latham calibration of Vega are presented. These scans contain more wavelength values than those given in previous papers in this series. The procedure of synthesizing u-b and b-y values from spectrophotometry is improved. Effective temperatures are found using the empirical calibration of Code and his colleagues and the fully line-blanketed solar composition model atmospheres of Kurucz.

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