(1) Institut für Astronomie und Astrophysik, Technische Universität Berlin, Sekr. PN 8-1, Hardenbergstrae 36, D-10623 Berlin, FRG;(2) Los Alamos National Laboratory, Group T-4, MS B268, 87545 Los Alamos, NM, USA
Abstract:
Synthetic brightness profiles resulting from consistent dynamical models for circumstellar dust shells around long-period variables are presented and discussed with respect to a corresponding observation of IRC +10216.