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Parravano, McKee & Hollenbach (2011)

San Diego State University

Abstract (paraphrased)

Assuming the disk IMF is universal and simple, the authors adopt a single smooth analytic form and constrain its parameters with integral observables (star counts, luminosities). The form approaches a power law at both ends — low-mass (ψmγ\psi \propto m^{\gamma}) and high-mass (ψmΓ\psi \propto m^{-\Gamma}) — joined smoothly, which they term the Smoothed Two-Power Law (STPL).

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References
  1. Parravano, A., McKee, C. F., & Hollenbach, D. J. (2011). An Initial Mass Function for Individual Stars in Galactic Disks. I. Constraining the Shape of the Initial Mass Function. The Astrophysical Journal, 726, 27. 10.1088/0004-637X/726/1/27