Precision Masses of the Low-Mass Binary System GJ 623

We have used aperture masking interferometry and adaptive optics (AO) at the Palomar 200 inch telescope to obtain precise mass measurements of the binary M dwarf GJ 623. AO observations spread over 3 yr combined with a decade of radial velocity measurements constrain all orbital parameters of the GJ 623 binary system accurately enough to critically challenge the models. The dynamical masses measured are m sub(1) = 0.371 plus or minus 0.015 M [unk] (4%) and m sub(2) = 0.115 plus or minus 0.0023 M [unk] (2%) for the primary and the secondary, respectively. Models are not consistent with color and mass, requiring very low metallicities.