M - L relations for rapid and slow rotators

Oleg Yu. Malkov
2006 Proceedings of the International Astronomical Union  
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.
doi:10.1017/s1743921307010253 fatcat:5vanjauo7bdxflpr7rlso5loqu