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Astron. Astrophys. 326, 1069-1075 (1997)

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Appendix A

The equivalent widths (in mA) for all the lines measured in this programme are detailed in Tables 9 and 10. In Table 10 the log gf values used in the analysis are given in column 4, with the associated references in column 5. The only log gf values that needed adjusting were ZrII 4772.31 and 5112.28. These were changed by -2.25 and -1.39, respectively, to bring the abundances due to these lines up to the average abundances from the other ZrII lines for the stars in M13.

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© European Southern Observatory (ESO) 1997

Online publication: April 8, 1998
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