Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60.1208k&link_type=abstract
(Astronomicheskii Zhurnal, vol. 60, Nov.-Dec. 1983, p. 1208-1216) Soviet Astronomy (ISSN 0038-5301), vol. 27, Nov.-Dec. 1983, p.
Astronomy and Astrophysics
Astronomy
4
Astrometry, Binary Stars, Orbital Elements, Stellar Motions, Celestial Mechanics, Orbital Mechanics, Radial Velocity, Secular Variations, Stellar Mass, Stellar Parallax
Scientific paper
The AMP method of obtaining a visual double star orbit yields two orbits satisfying the initial data when applied to a short arc. The method is proposed and investigated using individual old observations to choose the single solution and to estimate the value of the sum of component masses and the relative radial velocity. The orbit of the star ADS 9031, obtained by the new method from the 17-year series of observations, coincides well with the orbit obtained by Strand. The new orbit of the star 61 Cyg, determined from the 16-year series of observations, is calculated. It satisfies all the observations of the years 1834 - 1974.
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