Determination of the effective temperatures OF B, A, and F stars of luminosity classes III V from the slope of the spectrum in the Balmer continuum

Details Determination of the effective temperatures OF B, A, and F stars of luminosity classes III V from the slope of the spectrum in the Balmer continuum Determination of the effective temperatures OF B, A, and F stars of luminosity classes III V from the slope of the spectrum in the Balmer continuum

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap.....37..124s&link_type=abstract

Astrophysics, Volume 37, Issue 2, pp.124-129

Astronomy and Astrophysics

Astrophysics

Scientific paper

A new method is proposed for the determination of effective temperatures, which is based on the linear relationship between the slope of the spectrum in the Balmer continuum and the effective temperatures for B, A, and F stars of luminosity classes III V. Comparison of the effective temperatures found by this method and those found by other authors shows no systematic differences in the stellar temperatures.

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