Spectrophotometry of B, A, and F stars

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

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...222..547a&link_type=abstract

Astrophysical Journal, Part 1, vol. 222, June 1, 1978, p. 547-555.

Astronomy and Astrophysics

Astrophysics

62

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

Scientific paper

Energy distributions of 33 normal B, A, and F stars for wavelengths 3300-7100 are given that are consistent with the Hayes-Latham calibration of Vega. The derived upper limit on the photometric accuracy using a comparison of observed and synthetic u-b and b-y indices is 0.010 mag and 0.008 mag, respectively. Effective temperatures found using empirical calibrations agree with those derived using fully line-blanketed model atmospheres. Effective temperatures are found for selected spectral types.

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