Comment on the Radius of the Cooler Component of the Eclipsing RS CVn Binary CF Tuc (HD 5303)

Details Comment on the Radius of the Cooler Component of the Eclipsing RS CVn Binary CF Tuc (HD 5303) Comment on the Radius of the Cooler Component of the Eclipsing RS CVn Binary CF Tuc (HD 5303)

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ibvs.5007....1c&link_type=abstract

Information Bulletin on Variable Stars, 5007, 1.

Computer Science

1

Spectroscopy, Photometry

Scientific paper

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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