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Fig. 12

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Probability density that an AGB star of initial stellar mass M and metallicity Z contributes to the current populations of stardust for various grains in the ISM of the LMC. The adopted time scales of dust destruction in the ISM are 0.8 Gyr for silicate grains and 1.1 Gyr for carbonaceous, SiC grains, and iron grains.

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