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We present low-resolution spectroscopy of newly-discovered candidatecompanions to three stars in the Solar Neighbourhood. All three companions areM dwarfs, with spectral types ranging from M4 to M9.5. In two cases, G85-55`B'(M6) and G87-9`B' (M4), we have circumstantial evidence from spectroscopy,photometry and limited astrometry that the systems are physical binaries; inthe third, G216-7B (M9.5), comparison of POSS II IIIaF plate material and the2MASS image indicates common proper motion. The primary star in this system,G216-7A (M0), appears itself to be an unresolved, nearly equal-mass binary. Allthree low-mass companions are highly likely to be stellar in nature, althoughG216-7B lies very close to the hydrogen-burning limit.Comment: Accepted for publication in PASP; 21 pages, 6 figure

Three Newly Discovered M‐Dwarf Companions of Solar Neighborhood Stars