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

Details Temperatures from the log G - log M diagram for Algol-type binaries Temperatures from the log G - log M diagram for Algol-type binaries

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.169..121g&link_type=abstract

(IAU, European Regional Astronomy Meeting on New Windows to the Universe, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics a

Astronomy and Astrophysics

Astrophysics

7

Eclipsing Binary Stars, Main Sequence Stars, Stellar Evolution, Stellar Temperature, Cool Stars, Hot Stars, Late Stars, Stellar Models, Subgiant Stars

Scientific paper

The behavior 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. 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.

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