2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/4856We describe our method to construct line blanketed NLTE model atmospheres for hot stars. We employ the Accelerated Lambda Iteration and use statistical methods to deal with metal line blanketing.12 pages, To be published in: Modelling of Stellar Atmospheres, N.E. Piskunov, W.W. Weiss, D.F. Gray, eds., Proc. IAU Symp. 210Astrophysicstext