On the determination of double star orbits

Details On the determination of double star orbits On the determination of double star orbits

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..119e&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

5

Astrometry, Double Stars, Orbit Calculation, Orbital Elements, Stellar Motions, Astronomical Coordinates, Celestial Mechanics, Convergence, Power Series

Scientific paper

First-order and second-order derivatives are used in the development of the appropriate condition equations in order to improve the convergence of the determination of the orbital elements of visual binaries. A critique of the power-series methods is considered. To improve the accuracy of the orbit used as first approximation, the Kowalsky-Seeliger algorithm (Heintz, 1971) is modified.

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