Fig. 13
Mass functions of the subregions IRS4, IRSN3 and IRSN4. Power laws are fitted to the MFs above 0.5 M⊙ (solid lines) and for IRSN3 an additional power-law is fitted to the lower-mass end (0.06−0.5 M⊙). Overplotted is also the log-normal system MF representation of Chabrier (2005, dotted line).
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