Abstract
We discuss several categories of models which may explain the IMF, including the possible role of turbulence and magnetic fields.
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Basu, S. (2005). Turbulence Andmagnetic Fields in Clouds. In: Corbelli, E., Palla, F., Zinnecker, H. (eds) The Initial Mass Function 50 Years Later. Astrophysics and Space Science Library, vol 327. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-3407-7_84
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DOI: https://doi.org/10.1007/978-1-4020-3407-7_84
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