Fractional yields inferred from halo and thick disk stars (Serb. Astron. J. - 187 (2013), 19)

Abstract

Due to a wrong sign in a computer code, theoretical yield ratios have been recalculated. Related changes affect only Figs. 12-13, where theoretical yield ratios are represented as vertical bands. The correct figures are provided and differences with respect to the earlier version are mentioned. Minor corrections are also shown.

Keywords

• galaxy: evolution
• galaxy: formation
• stars: evolution
• stars: formation