The period distribution of eclipsing and spectroscopic binary systems. I

Details The period distribution of eclipsing and spectroscopic binary systems. I The period distribution of eclipsing and spectroscopic binary systems. I

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..54..389f&link_type=abstract

Astrophysics and Space Science, vol. 54, no. 2, Apr. 1978, p. 389-406. Research sponsored by the Consiglio Nazionale delle Rice

Astronomy and Astrophysics

Astrophysics

12

Binary Stars, Eclipsing Binary Stars, Star Distribution, Stellar Evolution, Density Wave Model, Least Squares Method, Logarithms, Statistical Analysis

Scientific paper

The period distribution of eclipsing and spectroscopic binary systems was analysed by various methods to take into account selection effects on observational data, with the purpose of deriving the actual distribution curve. The discussion of results shows the presence of some secondary maxima in the distribution which are probably of a nonstatistical character. They could be regarded as an indirect clue to the discrete nature of the star formation process, according to the spiral density wave theory of galactic evolution by Lin et al. (1969).

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