Reexamination of the mass-radius relation of main sequence in binary systems

Details Reexamination of the mass-radius relation of main sequence in binary systems Reexamination of the mass-radius relation of main sequence in binary systems

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pbeio..12...38z&link_type=abstract

Beijing Astronomical Observatory, Publications, March 1989, p. 38-46.

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2

Binary Stars, Line Spectra, Main Sequence Stars, Radii, Stellar Mass, Stellar Evolution, Stellar Models, Stellar Systems

Scientific paper

The mass-radius relation of the main sequence was reexamined using 171 components of 88 double-lined detached binary systems with well determined absolute dimensions and masses. Empirical relations for the ZAMS were obtained and compared with the theoretical models. The positions of the other 27 semidetached binaries in the log M - log R diagram are also discussed.

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