Temperatures from the log G-log M diagram for algol-type binaries

DOI: 
10.1007/BF00640697
Publication date: 
01/07/1990
Main author: 
García J.M.
IAA authors: 
Giménez A.
Authors: 
García J.M., Giménez A.
Journal: 
Astrophysics and Space Science
Publication type: 
Article
Volume: 
169
Pages: 
121-124
Number: 
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.
Database: 
WOK
SCOPUS
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/1990Ap&SS.169..121G/abstract
ADS Bibcode: 
1990Ap&SS.169..121G
Keywords: