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Refining the Orbit of Visual Double Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
An iterative method of refining the orbital parameters of visual double stars was described. The sum of the least-square differences is minimized by the Levenberg-Marquardt method. The application to two examples was described, including one highly inclined orbit, ADS 8862 = Hussey 664 (i = 94.3 degrees).
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- Part II Observational Methods
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- Copyright © Springer-Verlag 1988