Abstract
Most stars will experience episodes of substantial mass loss at some point in their lives. For very massive stars, mass loss dominates their evolution, although the mass loss rates are not known exactly, particularly once the star has left the main sequence.
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Arthur, S. (2007). Wind-Blown Bubbles around Evolved Stars. In: HARTQUIST, T., PITTARD, J., FALLE, S. (eds) Diffuse Matter from Star Forming Regions to Active Galaxies. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5425-9_10
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