Fig. 16
Simple sketch of the orbits of HR 10-A and -B around the centre of mass of the system plotted at scale as they are observed (top) and deprojected onto a plane using the value of the inclination, i, from Table 5. The stars have been located at the corresponding pericentres, i.e. the points where the distance between components A and B is a minimum (~ 2.39 au).
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