Synthetic spectra and mass determination of the brown dwarf Gliese 229B

We present preliminary nongray model atmospheres and interiors for cool brown dwarfs. The resulting synthetic spectra are compared to available spectroscopic and photometric observations of the coolest brown dwarf yet discovered, G1 229B (Nakajima et al.). Despite the grainless nature of the present models, we find that the resulting synthetic spectra provide an excellent fit to most of the spectral features of the brown dwarf. We confirm the presence of methane absorption and the substellar nature of G1 229B. These preliminary models set an upper limit for the effective temperature of 1000 K. We also compute the evolution of brown dwarfs with solar composition and masses from 0.02 to 0.065 M(.). While uncertainties in the age of the system yield some indeterminateness for the mass of G1 229B, the most likely solution is m approximate to 0.04 - 0.055 M(.). In any case, we can set an upper limit m = 0.065 M(.) for a very unlikely age, t = 10 Gyr.