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Fig. 2
Dissipated power as a function of time for a fast shell of material (Γ ≈ 200) that decelerates into the external medium and is eventually overtaken by a slower outflow, where Γ = 20. Results are shown for a uniform medium of density n = 30 cm-3 (red) and a stellar wind with A∗ = 2.4 (blue).
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