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- W1983645012 abstract "Abstract We have constructed three-dimensional hydrodynamical models to simulate the impact of massive star feedback, via winds and SNe, on inhomogeneous molecular material left over from the formation of a massive stellar cluster. We are studying the timescales for the molecular material to be removed from the environment of a massive stellar cluster and the mass and energy fluxes into the wider environment." @default.
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- W1983645012 date "2012-08-01" @default.
- W1983645012 modified "2023-09-27" @default.
- W1983645012 title "Stellar wind and supernova feedback from massive stars" @default.
- W1983645012 doi "https://doi.org/10.1017/s1743921314012289" @default.
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