M - L relations for rapid and slow rotators

Details M - L relations for rapid and slow rotators M - L relations for rapid and slow rotators

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..213m&link_type=abstract

Highlights of Astronomy, Volume 14, p. 213-213

Astronomy and Astrophysics

Astronomy

Binaries: Eclipsing

Scientific paper

Comparing the radii of eclipsing binaries components and single stars we have found a noticeable difference between observational parameters of B0V - G0V components of eclipsing binaries and those of single stars of the corresponding spectral type. This difference was confirmed by re-analyzing the results of independent investigations published in the literature.

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