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Processes controlling the initial mass function: interstellar turbulence and magnetic fields
Published online by Cambridge University Press: 03 August 2017
Abstract
The observed flattening of the initial stellar mass function at low mass can be accounted for in terms of the different interstellar cloud size-mass scaling and different ambipolar diffusion time scaling for small, thermally-supported clouds and larger clouds supported primarily by turbulent pressure.
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- Copyright © Kluwer 1991