A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
M - L relations for rapid and slow rotators
2006
Proceedings of the International Astronomical Union
Preserved Fulltext
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