The optical mass-luminosity relation at the end of the main sequence (0.08-0.20 M-circle dot)

The empirical mass-luminosity relation at M-V is presented for stars with m asses 0.08-0.20 M-. based upon new observations made with Fine Guidance Sen sor 3 on the Hubble Space Telescope. The targets are nearby, red dwarf mult iple systems in which the magnitude differences are typically measured to /-0.1 mag or better. The M-V values are generated using the best available parallaxes and are also accurate to +/-0.1 mag, because the errors in the m agnitude differences are the dominant error source. In several cases this i s the first time the observed sub-arcsecond multiples have been resolved at optical wavelengths. The mass-luminosity relation defined by these data re aches to M-V = 18.5 and provides a powerful empirical test for discriminati ng the lowest mass stars from high-mass brown dwarfs at wavelengths shorter than 1 mu m.