Absolute parameters of stars in semidetached eclipsing binary systems

Details Absolute parameters of stars in semidetached eclipsing binary systems Absolute parameters of stars in semidetached eclipsing binary systems

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..584b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, June 1985, p. 584-590.

Astronomy and Astrophysics

Astronomy

14

Eclipsing Binary Stars, Mass To Light Ratios, Stellar Mass, Astronomical Catalogs, Mass Ratios, Stellar Luminosity

Scientific paper

A number of questions concerning the absolute parameters of stars in semidetached binary systems are addressed. Consideration is given to: similarities between Algol-type binaries and unevolved detached binaries with respect to the mass-luminosity law; and the single-line classical Algol candidates with known mass functions and photometric solutions for mass ratio. It is shown that the validity of the mass luminosity-law cannot be verified for individual Algol-type binaries though it does hold well on average; and (2), the existence of a definite class of sd-binaries not containing a proportion of significantly undersize types is apparent. The conclusions are found to be in general agreement with the observations of Hall and Neff (1979).

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