The primary purpose of this paper is to describe an efficient method of computing rotation-broadening effects allowing for the full limb-distance variation of both the continuum...
This report presents a computer program for the calculation of a non-LTE model atmosphere of early-type stars subject to the constraints of radiative, hydrostatic, and...
We investigate the relation between 1D atmosphere models that rely on the mixing length theory and models based on full 3D radiative hydrodynamic (RHD) calculations to describe...
We have assembled an atlas of line profiles of the Paschen Delta (P-{delta}) line at 10049{AA} for the use of stellar modelling. For a few stars we have substituted the Paschen...
