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Cited article:

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Three-component modelling of C-rich AGB star winds – V. Effects of frequency-dependent radiative transfer including drift★

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Monthly Notices of the Royal Astronomical Society 499 (2) 1531 (2020)
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The resonant drag instability (RDI): acoustic modes

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Observing and modeling the dynamic atmosphere of the low mass-loss C-star R Sculptoris at high angular resolution

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Three-component modelling of C-rich AGB star winds - IV. Revised interpretation with improved numerical descriptions

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Monthly Notices of the Royal Astronomical Society 385 (1) 215 (2008)
https://doi.org/10.1111/j.1365-2966.2007.12644.x

A Self-Consistent Determination of the Temperature Profile and The Magnetic Field Geometry in Winds of Late-Type Stars

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Infrared photometry and evolution of mass-losing AGB stars

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Astronomy & Astrophysics 445 (3) 1069 (2006)
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On the magnetic structure and wind parameter profiles of Alfvén wave driven winds in late-type supergiant stars

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Monthly Notices of the Royal Astronomical Society 368 (3) 1145 (2006)
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The Effects of Alfven Waves and Radiation Pressure in Dusty Winds of Late‐Type Stars. II. Dust‐Cyclotron Damping

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The case for asymmetric dust around a C-rich asymptotic giant branch star

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Monthly Notices of the Royal Astronomical Society 346 (3) 878 (2003)
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