Astron. Astrophys. 322, 1026-1026 (1997)
Abundance analysis of roAp stars
II. HD 203932
1 Inst. of Astronomy, Univ. Vienna, Türkenschanzstr.
17, A-1180 Vienna, Austria (E-MAIL:
2 European Southern Observatory, Santiago, Chile
Received 26 March 1996 / Accepted 9 August 1996
The correct Fig. 5 and Fig. 6 are:
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 = 7450 K.
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 = 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