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

R. Caimmi
2014 Serbian Astronomical Journal  
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.
doi:10.2298/saj1488099e fatcat:crjtp7tflnd3zlo6u3bdqpmzxa