Close triple star systems

Details Close triple star systems Close triple star systems

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..137w&link_type=abstract

(Deutsche Forschungsgemeinschaft, Universitaet Bamberg, Universitaet Erlangen-Nuernberg, and Victoria University of Manchester,

Astronomy and Astrophysics

Astrophysics

Astrometry, Eclipsing Binary Stars, Light Curve, Orbital Elements, Stellar Motions, Three Body Problem, Triple Stars, Mass Ratios, Minima

Scientific paper

Triple-star systems, especially those in which one star has very small mass, are examined. Observations that provide information about the physical nature of close systems, in particular, changes of the period of orbital revolution, are discussed. It is shown that the detection and study of these changes is best obtained by observations of the precise times of light minima in eclipsing systems. Examples of work on period changes caused by a third companion are given.

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