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- W2088358051 abstract "A coalescence model using the observed properties of pre‐stellar condensations (PSCs) shows how an initially steep initial mass function (IMF) that might be characteristic of primordial cloud fragmentation can change into a Salpeter IMF or shallower IMF in a cluster of normal density after one dynamical time, even if the PSCs are collapsing on their own dynamical time. The model suggests that top‐heavy IMFs in some starburst clusters originate with PSC coalescence." @default.
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- W2088358051 date "2004-10-01" @default.
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- W2088358051 title "Variability in the stellar initial mass function at high mass: coalescence models for starburst clusters" @default.
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- W2088358051 doi "https://doi.org/10.1111/j.1365-2966.2004.08188.x" @default.
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