Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983lastr..97..189b&link_type=abstract
L'Astronomie (ISSN 0004-6302), vol. 97, April 1983, p. 189-195. In French.
Astronomy and Astrophysics
Astronomy
Binary Stars, Stellar Motions, Eccentric Orbits, Tables (Data)
Scientific paper
Historical measurements of components of binary star systems at times exhibit evidence for incompatible interpretations. A short period and strong eccentricity can equally be a long period with feeble eccentricity. Furthermore, measurements have been made indicating both direct and retrograde motions of the components. It has sometimes been found that the observations of contradicting evidence have been made of a second binary system near the system first measured. Note is taken of the objects ADS 1959 - A 1818, ADS 2051 - HU 539, ADS 5515 - A 512, ADS 5671 - BU 1022, ADS 6001 - A 1963, and ADS 7550 - A 2561, which may possibly be combinations of two or even three binary clusters observed at different times. Tables are presented of data thus far measured of each system.
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