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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Star formation model choice in galaxy simulations controls giant molecular cloud lifetimes, yielding 20-30 Myr with sink particles versus over 200 Myr with the gravo-thermo-turbulent prescription.
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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.
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From short-lived to long-lived clouds: impact of star formation models on giant molecular cloud evolution in simulations of an NGC 300-like galaxy
Star formation model choice in galaxy simulations controls giant molecular cloud lifetimes, yielding 20-30 Myr with sink particles versus over 200 Myr with the gravo-thermo-turbulent prescription.