Fig. 7 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. 7.

(a) Mass of the most massive core, and (b) mass at which the maximum of the histogram occurs as a function of M_s. Filled (open) squares denote results from SPH (TVD) runs. Solid lines represent least‐squares fits to the data, and m represents the slope of the fit. Note that, for each numeric scheme, the mass decreases as the M_s number increases.

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