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Fig. 2
Dynamical time tdyn of the material ejected from a stellar surface because of the over-Eddington luminosity. ΔM is the mass lost from the stellar core. Left panel shows the dynamical time required to reach 10 R⋆ from R⋆. Right panel shows the dynamical time required to reach 100 R⋆ from R⋆.
This figure is made of several images, please see below:
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