SIMulation pour Etoiles Chaudes Actives (SIMECA)
This SIMECA code, based on a radiative wind model, computes hydrogen line profiles, Spectral Energy Distributions (SEDs) and intensity maps which can be directly compared to high angular resolution observations. This code is dedicated to the modeling of active hot stars, mainly Be, B[e], LBV, WR and HAe/Be stars. It is possible to study the […]