Eclipsing binaries with light-time effect

Details Eclipsing binaries with light-time effect Eclipsing binaries with light-time effect

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990baicz..41..231m&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 41, no. 4, July 1990, p. 231-236.

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56

Eclipsing Binary Stars, Three Body Problem, Triple Stars, Kepler Laws, Periodic Variations

Scientific paper

Known cases of eclipsing binaries, the period changes of which can be explained by orbiting a common mass center with a third body, are reviewed. Only three systems, where the third-body periods are shorter than 4 years, are considered certain. In 12 other cases the light-time effect gives a fair explanation of their O-C plots, however, lacking other proofs of the third-body presence, they can be treated as probable cases only. Some parameters of these triple and multiple systems are discussed.

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