Astron. Astrophys. 324, 435-448 (1997)

Appendix

In Table 5, we give all the lines that we used in the analysis of our SMC K supergiants. The first four columns give respectively: the central wavelength of the line in , the element and its degree of ionization, the excitation potential in eV, the line transition probability in log scale (). Then we give for each of the six SMC stars, the equivalent width (in µÅ) and the resulting abundance ([M/H], normalized to the Sun) for the line. Asterisks surrounding the equivalent width means that the abundance was determined by fitting the line profile rather than using this equivalent width, due to a severe blend or to hyperfine structure of the line.

Table 5. Lines used in the analysis of our SMC K supergiants: (1) central wavelength of the line in Å, (2) element and its degree of ionization (1 for neutral and 2 for ionized species), (3) the excitation potential in eV, (4) line transition probability in log scale (); columns (5) through (14) give, for each of the six SMC stars, the equivalent width (in mÅ) and the resulting abundance ([M/H], abundance in log scale, normalized to the Sun) for the line.

© European Southern Observatory (ESO) 1997

Online publication: May 26, 1998

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