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Article Contents
1 Introduction and the problem of Mira sizes
2 Observations and data reduction
3 Photometric data
4 Data modeling
5 Results of the modeling
6 Comparison to other data
7 Radii, temperatures, pulsation and atmosphere
8 Discussion of the model - what is star and what is shell?
9 Conclusions
References
Online Material

List of tables
List of figures

Copyright ESO 2004
Published by EDP Sciences