Fig. 6.
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Initial stellar mass estimation of the aggregate candidate Pismis 5, Pismis 5A, and Pismis 5B, (a) QZ 1; (b) aggregate candidate composed of Alessi 43 and Collinder 197; (c) BH 56 (d); and NGC 2546; (e) based on the IMF model (Kroupa 2001). The histograms, which are fitted with IMFs of varied total mass, show the observed mass distribution.
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