Stellar wind termination shocks in massive clusters have structure determined solely by the surrounding cavity's density and pressure, enabling efficient modeling of arbitrary cluster ages and producing spherical shocks in 5 Myr old systems.
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How interacting winds shape the mechanical feedback of massive star clusters over millions of years
Stellar wind termination shocks in massive clusters have structure determined solely by the surrounding cavity's density and pressure, enabling efficient modeling of arbitrary cluster ages and producing spherical shocks in 5 Myr old systems.