All Tables

Table 1: Log of UVES observations of HD 133792.
Table 2: Atmospheric abundances in the Ap star HD 133792 with the error estimates based on n measured lines. Abundances in the solar atmosphere and in the evolved Ap star HD 204411 are given for comparison.
Table 3: A list of spectral lines used for the stratification calculations. The columns give the ion identification, central wavelength, the excitation potential (in eV) of the lower level, oscillator strength ( $\log~{gf}$ ), the Stark damping constant ("appr'' marks lines for which the classical approximation was used), and the reference for oscillator strength.