Fig. 9.

Yields of intermediate-mass stars of different metallicities. Values for Z = 10−5 cases are shown in thin blue lines for the models calculated with VW93 from Campbell & Lattanzio (2008; 0.85, 1, 2 and 3 M⊙). Our models computed with VW93 (between 3 and 7 M⊙) are shown in black solid lines, and those with Blo95 are shown in black dashed lines. Values in orange correspond to the Z = 10−4 models from Karakas (2010; 1 to 6 M⊙) and (Doherty et al. 2014b; 7 and 7.5 M⊙). Values in green correspond to the Z = 10−3 models from Fishlock et al. (2014; 1 to 6 M⊙) and Doherty et al. (2014b; 7 and 7.5 M⊙).
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