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The chaotic winds of AGB stars: Observation meets theory

ESO Astrophysics Symposia (2008) 2008 181-185
DOI: 10.1007/978-3-540-74256-2_20
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Abstract

Spherically symmetric (1D) and axisymmetric (2D) dynamical simulations for dust-driven winds of carbon stars are presented which aim at a qualified interpretation of interferometric image and visibility data. © 2007 Springer.

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Woitke, P., & Quirrenbach, A. (2008). The chaotic winds of AGB stars: Observation meets theory. In ESO Astrophysics Symposia (Vol. 2008, pp. 181–185). https://doi.org/10.1007/978-3-540-74256-2_20

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