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Astron. Astrophys. 322, 1026-1026 (1997)

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Abundance analysis of roAp stars

II. HD 203932

M. , Gelbmann 1, F. , Kupka 1, W. , W. , Weiss 1, G. and Mathys 2

1 Inst. of Astronomy, Univ. Vienna, Türkenschanzstr. 17, A-1180 Vienna, Austria (E-MAIL: last_name@galileo.ast.univie.ac.at)
2 European Southern Observatory, Santiago, Chile

Received 26 March 1996 / Accepted 9 August 1996

The correct Fig. 5 and Fig. 6 are:

[FIGURE] Fig. 5. Confirmation of the effective temperature of HD 203932: Abundances of 41 Fe I (diamonds) and 28 Fe II lines (crosses) are plotted versus the lower energy level for [FORMULA] = 7450 K.
[FIGURE] Fig. 6. Confirmation of the microturbulent velocity. Abundances versus equivalent width of 41 Fe I (diamonds) and 28 Fe II lines (crosses) are plotted for [FORMULA] = 0.0 km s-1.

The wrong figures are based on a different sample of iron lines and do not distinguish between Fe I (diamonds) and Fe II (crosses).

© European Southern Observatory (ESO) 1997

Online publication: June 5, 1998