Distribution of eclipsing binaries with respect to mass of components and major axis of orbit

Details Distribution of eclipsing binaries with respect to mass of components and major axis of orbit Distribution of eclipsing binaries with respect to mass of components and major axis of orbit

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7..488k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Aug. 1981, p. 488-492.) Soviet Astronomy Letters, vol. 7, July-Aug. 1981, p. 269-271

Astronomy and Astrophysics

Astronomy

11

Eclipsing Binary Stars, Orbital Elements, Star Distribution, Stellar Mass, Stellar Motions, Stellar Evolution, Stellar Luminosity, Stellar Mass Accretion, Stellar Mass Ejection, Stellar Spectrophotometry

Scientific paper

The mass distribution of the primary component and orbit major semiaxis a is investigated for the case of 482 eclipsing binaries with primaries of a known spectral type and luminosity class. It is determined that the number of stars per unit interval of log a is deficient by comparison with wider systems, through consideration of the parameter domain where log (primary component mass/solar mass) is greater than about 0.45, and log a/solar radius is less than about 1.0.

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