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. 15.

todmor RV curves of UCAC4 355−020729 as a function of the orbital phase, along with their best-fitting models. The blue and red circles correspond to the primary and secondary components, respectively, while the crosses indicate data points not used in the fit. The residuals from the fit are shown in the bottom panels.

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