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arXiv · astro-ph/0410080

Feedback and the Initial Mass function

Joseph Silk
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Abstract

I describe a turbulence-inspired model for the stellar initial mass function which includes feedback and self-regulation via protostellar outflows. A new aspect of the model provides predictions of the star formation rate in molecular clouds and gas complexes. A similar approach is discussed for self-regulation on kiloparsec scales via supernova input, and an expression is presented for the global star formation rate that depends on the turbulent pressure of the interstellar medium.

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Joseph Silk. 2004-10-04. Feedback and the Initial Mass function. https://doi.org/10.1007/978-1-4020-3407-7_81

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