Fig. 2 from The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function

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The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function

Authors: Javier Ballesteros-Paredes, Adriana Gazol, Jongsoo Kim, Ralf S. Klessen, Anne-Katharina Jappsen, and Epimenio Tejero

Ballesteros‐Paredes et al. 2006 The Astrophysical Journal 637 384.

Provider: AAS Journals

Caption: Fig. 2.

Energy spectrum for each simulation. The solid lines correspond to SPH simulations and the dotted lines to TVD simulations. The dashed lines have a slope of −2 and ﹩-5/ 3﹩.

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