Clumps in stellar winds

Vink, J. S.

We discuss the origin and quantification of wind clumping and mass–loss rates (Ṁ), particularly in close proximity to the Eddington (Γ) limit, relevant for very massive stars (VMS). We present evidence that clumping may not be the result of the line-deshadowing instability (LDI), but that clumps are already present in the stellar photosphere.

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Vink, J. S.: Clumps in stellar winds. 2014. Copernicus Publications.

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Rechteinhaber: J. S. Vink

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