  Based on detailed 2D radiation hydrodynamics (RHD) simulations, we have
investigated the effects of photospheric temperature inhomogeneities induced by
convection on spectroscopic determinations of the lithium abundance.
Computations have been performed both for the solar case and for a metal-poor
dwarf. NLTE effects are taken into account, using a five-level atomic model for
LiI. Comparisons are presented with traditional 1D models having the same
effective temperature and gravity. The net result is that, while LTE results
differ dramatically between 1D and 2D models, especially in the metal-poor
case, this does not remain true when NLTE effects are included: 1D/2D
differences in the inferred NLTE Li abundance are always well below 0.1 dex.
The present computations still assume LTE in the continuum. New computations
removing this assumption are planned for the near future.
