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Fig. 19


Orbital elements as function of eccentricity for all solutions with out of 5 000 000 runs of our LSMC fit of the PZ Tel B astrometric data. From left to right and from top to bottom are represented the semi-major axis, inclination, longitude of the ascending node, argument of periastron, and time at periastron passage. Logarithmic density of solutions is indicated by color.

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