A New Calibration of Wesselink's Correlation for the Determination of Stellar Radii

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

By means of a new homogeneous set of data from 34 double-lined detached
systems, we have recalibrated the colour-surface brightness correlation
in the interval -0.3≤(B-V)o≤0.95. A comparison is
made with Wesselink's calibration. We find that Wesselink's method can
provide a good estimate of the stellar radii.

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