Fig. 1
Dust masses for carbonaceous, silicate, SiC and iron grains condensed by AGB stars, taken from Zhukovska et al. (2008), shown by plus symbols and crosses for initial stellar metallicities Z = 0.001 and Z = 0.008, respectively, and taken from Ventura et al. (2012b, solid lines) for Z = 0.001 and Ventura et al. (2012a, dashed lines) for Z = 0.008.
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