par Rau, Gioia;Paladini, Claudia ;Hron, Josef;Aringer, Bernhard;Eriksson, Kjell;Groenewegen, Martin A. T.;Nowotny, Walter
Référence Proceedings of the International Astronomical Union, 11, A29B, page (160-161)
Publication Publié, 2015
Article révisé par les pairs
Résumé : We compare in a systematic way spectrometric, photometric and mid-infrared (VLTI/MIDI) interferometric measurements with different types of model atmospheres. Self-consistent dynamic model atmospheres in particular were used to interpret in a consistent way the dynamic behavior of gas and dust. The results underline how the joint use of different kind of observations, as photometry, spectroscopy and interferometry, is essential to understand the atmospheres of pulsating C-rich AGB stars. The sample of C-rich stars discussed in this work provides crucial constraints for the atmospheric structure.