2711 20160701171709.0 ASTROimport-868 Rau, G. 2015 Into the Modelling of RU Vir We present an attempt to model the atmosphere of the carbon-rich Mira star RU Vir, using different techniques including spectroscopy, photometry, and interferometry. A radiative transfer code and hydrostatic model atmospheres were used for a preliminary study. To investigate the dynamic processes happening in RU Vir, dynamic model atmospheres were compared to new MIDI/VLTI observations obtained in April 2014, and SiC opacities were added. Hron, J. Paladini, C. Eriksson, K. Aringer, B. Groenewegen, M. A. T. Mecina, M. Why Galaxies Care about AGB Stars III: A Closer Look in Space and Time 497 2015 137 http://esoads.eso.org/abs/2015ASPC..497..137R published in NONREF