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Fig. 8
Comparison of the orbits of Adibekyan et al. (2012) stars projected in the R−z plane for Model I (top panel), Model II (middle panel), and Model A&S (bottom panel). Only one out of ten stars of those in the Adibekyan et al. (2012) sample is shown. Different colours correspond to different stars.
This figure is made of several images, please see below:
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