Vol 25, No 2

Core Mass Function in View of Fractal and Turbulent Filaments and Fibers

Xunchuan Liu (刘训川), Tie Liu, Xiaofeng Mai, Yu Cheng, Sihan Jiao, Wenyu Jiao, Hongli Liu and Siju Zhang

Abstract

We propose that the core mass function (CMF) can be driven by filament fragmentation. To model a star-forming system of filaments and fibers, we develop a fractal and turbulent tree with a fractal dimension of 2 and a Larson's law exponent (β) of 0.5. The fragmentation driven by convergent flows along the splines of the fractal tree yields a Kroupa-IMF-like CMF that can be divided into three power-law segments with exponents α = −0.5, −1.5, and −2, respectively. The turnover masses of the derived CMF are approximately four times those of the Kroupa IMF, corresponding to a star formation efficiency of 0.25. Adopting β = 1/3, which leads to fractional Brownian motion along the filament, may explain a steeper CMF at the high-mass end, with α = −3.33 close to that of the Salpeter IMF. We suggest that the fibers of the tree are basic building blocks of star formation, with similar properties across different clouds, establishing a common density threshold for star formation and leading to a universal CMF.

Keywords

stars: formation – stars: kinematics and dynamics – turbulence – stars: luminosity function, mass function – ISM: clouds

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