The CARMENES search for exoplanets around M dwarfs - Spectroscopic orbits of nine M-dwarf multiple systems, including two triples, two brown dwarf candidates, and one close M-dwarf–white dwarf binary

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Fig. 17.

Best fit to the todmor RVs of UU UMi as a function of time. Blue and red correspond to the primary and secondary components, respectively. Circular and triangular symbols correspond to the RVs from CARMENES and CAFE, respectively. The residuals from the best fit are shown in the bottom panels.

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