Citation: D. Schaerer et W. Schmutz, HYDRODYNAMIC ATMOSPHERE MODELS FOR HOT LUMINOUS STARS .2. METHOD AND IMPROVEMENTS OVER UNIFIED MODELS, Space science reviews, 66(1-4), 1993, pp. 173-177
Citation: A. Dekoter et al., A FAST NON-LTE CODE FOR EXPANDING ATMOSPHERES - A TEST OF THE VALIDITY OF THE SOBOLEV APPROXIMATION, Astronomy and astrophysics, 277(2), 1993, pp. 561-577