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