A simple model for the complex structure of moving atmospheric shells in Oe and Be stars. The example of HD 152408, some first conclusions. JENAM 2000, May 29-June 3, 2000 Moscow, Russia. 

Abstract

    In this paper we present the application for the star HD 152408 of the atmospheric model first announced by Danezis et al. at the 1998 JENAM in Prague and also submitted in Symposium 205 of the I.A.U. 
    We also present the initial conclusions that are supported by the results of this process. This work is a part of a wider study of the gas shells of early type stars, in order to classify them systematically.