Abstract
The ingredients necessary for a consistent description of dust forming atmospheres around pulsating stars are addressed and the results of corresponding hydrodynamical model calculations are compared with respective observations
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Winters, J.M. (2003). Confronting Consistent Dust Shell Models with Observations of Long-Period Variable Stars. In: Nakada, Y., Honma, M., Seki, M. (eds) Mass-Losing Pulsating Stars and their Circumstellar Matter. Astrophysics and Space Science Library, vol 283. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0139-7_31
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DOI: https://doi.org/10.1007/978-94-010-0139-7_31
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