Brγequivalent width as a function of near-IR color excess E(K_s−L′) . Filled symbols show accretion detections, open symbols are upper limits of W_Brγ . Primaries and secondaries are denoted by circles and diamonds. Stars to the right of the dotted line have significant K_s−L′excess. Targets without veiling measurement can have larger W_Brγthan shown here since the correction factor (1 + r_K) could not be applied; they are marked with arrows.