The mass-radius relation in binary systems

Details The mass-radius relation in binary systems The mass-radius relation in binary systems

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.114..259g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 114, no. 2, Sept. 1985, p. 259-269.

Statistics

Computation

14

Binary Stars, Main Sequence Stars, Radii, Stellar Mass, Astrometry, Computational Astrophysics, Logarithms, Stellar Models

Scientific paper

The mass-radius relation is determined for main-sequence stars from
observational data of well-detached binary systems. The results are
compared to previous empirical relations and their application to the
study of the light curves of eclipsing binaries is studied. A comparison
with theoretical main-sequence models has been carried out.

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