Journal:
Astrophysics and Space Science
Abstract:
The behaviour of the primary and secondary components in a sample of double-lined Algol-type eclipsing binaries in the log g-log Te diagram is analyzed. Our results indicate that the hotter components behave like normal Main-Sequence stars while the effect of irradiation may partly explain the 'overluminosity' of the cool components. © 1990 Kluwer Academic Publishers.
URL:
https://ui.adsabs.harvard.edu/#abs/1990Ap&SS.169..121G/abstract