Spectrophotometry of B, A, and F stars. II

Details Spectrophotometry of B, A, and F stars. II Spectrophotometry of B, A, and F stars. II

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apjs...43..491a&link_type=abstract

Astrophysical Journal Supplement Series, vol. 43, Aug. 1980, p. 491-499.

Astronomy and Astrophysics

Astrophysics

33

A Stars, B Stars, Early Stars, F Stars, Stellar Spectrophotometry, Accuracy, Spectral Energy Distribution, Stellar Temperature, Tables (Data)

Scientific paper

Optical region energy distributions of 35 normal B, A, and F stars are presented consistent with the Hayes-Latham calibration of Vega. Upper limits on the photometric accuracy are derived by a comparison of observed and synthesized u-b and b-y indices for each observer. Effective temperatures are found using the empirical calibration of Code et al. (1976) and the fully line blanketed solar composition model atmospheres of Kurucz (1979).

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