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2000IBVS.5007....1C - IAU Inform. Bull. Var. Stars, 5007, 1 (2000/December-0)
Comment on the radius of the cooler component of the eclipsing RS CVn binary CF Tuc (HD 5303).
COATES D.W., THOMPSON K. and INNIS J.L.
Abstract (from CDS):
The value of rotational v sin i for the cooler star in the eclipsing RS CVn binary CF Tuc deduced from high-resolution spectroscopy and least-squares deconvolution by Donati et al. (1997) appears to be too high when compared to the radius obtained from the light-curve solution. We suggest that this case be studied further.
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