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Remarks on Orbits and Dynamical Parallaxes
Published online by Cambridge University Press: 14 August 2017
Extract
In connection with statements made at the preceding session, some results presented at the Nice Conference on systematic and random errors affecting the elements a and P as well as a3/P2 may be recalled. If many orbits have been calculated for one binary, it is instructive to plot log P, log a, and log a3/P2 versus log Δt/P where Δt is the time interval covered by observations. As a general rule, when Δt ≃ P the systematic trends vanish, and the scatter of the plotted elements reaches a low value, not considerably changing thereafter. It may well be of interest, then, to have several orbits based on the same observations but computed by different authors and methods.
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- Session 2. Orbital Parameters
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- Copyright © The University of Toronto Press, Royal Astronomical society of Canada 1973