The photometric evolution of dissolving star clusters - II. Realistic models. Colours and M/L ratios

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Table 1:

The best-fit coefficients for Eq. (6). The middle column gives the coefficients for the low-mass end of the MF for masses $\le$ 0.3 $M_\odot$ . The right column gives the coefficients for masses >0.3 $M_\odot$ .
Coefficient	$m \le 0.3$ $M_\odot$	m > 0.3 $M_\odot$
a₁	-0.1345	0.08389
a₂	1.7986	1.9324
a₃	-1.8121	-0.4435
a₄	1.2181	0.734
b	3.215e-6	-1.4143e-5

The middle column gives the coefficients for the low-mass end of the MF for masses $\le$ 0.3 $M_\odot$ .
The right column gives the coefficients for masses >0.3 $M_\odot$ .

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