Orbits and masses in the multiple system LHS 1070 | Astronomy & Astrophysics (A&A)

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Fig. 6

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Distances between the three stars in the system as function of time. Here we assume that the stars stay on the Keplerian orbits derived in Sects. 3 and 4, i.e. we do not simulate the three-body problem posed by the triple system.

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