000002711 001__ 2711
000002711 005__ 20160701171709.0
000002711 037__ $$aASTROimport-868
000002711 100__ $$aRau, G.
000002711 245__ $$aInto the Modelling of RU Vir
000002711 260__ $$c2015
000002711 520__ $$aWe present an attempt to model the atmosphere of the carbon-rich Mira star RU Vir, using different techniques including spectroscopy, photometry, and interferometry. A radiative transfer code and hydrostatic model atmospheres were used for a preliminary study. To investigate the dynamic processes happening in RU Vir, dynamic model atmospheres were compared to new MIDI/VLTI observations obtained in April 2014, and SiC opacities were added. 
000002711 700__ $$a Hron, J.
000002711 700__ $$a Paladini, C.
000002711 700__ $$a Eriksson, K.
000002711 700__ $$a Aringer, B.
000002711 700__ $$a Groenewegen, M. A. T.
000002711 700__ $$a Mecina, M.
000002711 773__ $$c137$$pWhy Galaxies Care about AGB Stars III: A Closer Look in Space and Time$$v497$$y2015
000002711 85642 $$ahttp://esoads.eso.org/abs/2015ASPC..497..137R
000002711 905__ $$apublished in
000002711 980__ $$aNONREF