**Table 1:** Relative and absolute dust ISM feedback contribution fordifferent stellar component mass functions.
Stellar mass range	IMF	PDMF
$M_{\rm d}$ ( $M>8~M_{\odot}$ )	68%	1%
$M_{\rm d}$ ( $M<8~M_{\odot}$ )	32%	99%
$M_{\rm d\_total}$ ^a ( $M_{\odot }$ )	$7 \times 10^{7}$	$2 \times 10^{7}$

^a Assuming a total stellar population of $1 \times 10^{10}~M_{\odot}$ .

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