Detection of low eccentricity orbits - an analysis of nine massive spectroscopic binaries

Details Detection of low eccentricity orbits - an analysis of nine massive spectroscopic binaries Detection of low eccentricity orbits - an analysis of nine massive spectroscopic binaries

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91...95m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Feb.-Mar. 1979, p. 95-98. NSF-supported research.

Statistics

Computation

7

B Stars, Binary Stars, Eccentric Orbits, Stellar Spectrophotometry, Cosmic Noise, Detection, Eccentricity, Fourier Transformation, Mass Transfer, Signal Analysis

Scientific paper

The elements of nine single-lined, short-period, massive spectroscopic binaries are analyzed for significant orbital eccentricity. The Fourier transform formalism for computation of orbits is used to derive an estimator of significance for the observed eccentricity. Of the nine systems investigated, five are either probably or possibly in eccentric orbits.

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