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This article has an erratum: [https://doi.org/10.1051/0004-6361/201730725e]


Fig. 2

image

Best-fit orbit of C around B in the rest frame of B. The ascending and descending nodes are marked by the dash-dotted line and the periastron by the dashed line. The ellipses mark the errors of the observed positions, with red lines connecting the observed positions with the calculated orbit. The orbital motion is counter-clockwise, as depicted by the arrow.

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