Comparison of HD 160934 components with some PMS theoretical models (Baraffe et al. 1998, top left; Siess et al. 2000, top right; Tognelli et al. 2011, middle left; and Bressan et al. 2012, middle right; Baraffe et al. 2015, bottom left; and Choi et al. 2016, bottom right). For each model, isomasses (solid lines) and isochrones (dashed lines) are plotted. We highlight the nearest tracks available corresponding to our dynamical mass values. The theoretical masses are consistent with our dynamical estimates just at the extreme of their uncertainties.