All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=8.5cm,clip]{Gk081_f1.ps}\hspace*{5mm} \includegraphics[angle=-90,width=8.15cm,clip]{Gk081_f2.ps} \end{figure}$ Figure 1: Variations of $\langle B_z\rangle$ ( left panel), $W_\lambda/\langle W\rangle$ ( right top panel), and mean light in the Johnson B filter (taken from KM and references therein, right lower panel) of HD 24712, phased according to the adopted rotation period. The new MuSiCos data are represented by filled circles in both the $\langle B_z\rangle$ and $W_\lambda/\langle W\rangle$ frames. Open circles - Balmer-line magnetometer and $W_\lambda/\langle W\rangle$ data from Ryabchikova et al. (1997) (with $\langle B_z\rangle$ decreased by 400 G). Asterisks - $\langle B_z\rangle$ data from Mathys (1991) and Mathys & Hubrig (1997) and $W_\lambda/\langle W\rangle$ data from Bonsack (1979). Open squares - $\langle B_z\rangle$ data from Leone & Catanzaro (2004) and $W_\lambda/\langle W\rangle$ data from pulsational observations. Pluses (+) represent Preston's (1972) $\langle B_z\rangle$ measurements from TiCrFe lines.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{Gk081_f3.ps} \end{figure}$ Figure 2: HD 12098: mean longitudinal magnetic field ( top panel) and pulsation amplitudes (Girish et al. 2001) phased according to the 5.46 day rotation period. Uncertainties associated with the $\langle B_z\rangle$ measurements are about the same size as than the symbols.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{Gk081_f4.ps} \end{figure}$ Figure 3: HD 122970: longitudinal magnetic field variations with the rotational period 3.877 day (filled circles). One measurement from Hubrig et al. (2004) is shown by open square.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{Gk081_f3.ps} \end{figure}$	Figure 2: HD 12098: mean longitudinal magnetic field ( top panel) and pulsation amplitudes (Girish et al. 2001) phased according to the 5.46 day rotation period. Uncertainties associated with the $\langle B_z\rangle$ measurements are about the same size as than the symbols.
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$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{Gk081_f4.ps} \end{figure}$	Figure 3: HD 122970: longitudinal magnetic field variations with the rotational period 3.877 day (filled circles). One measurement from Hubrig et al. (2004) is shown by open square.
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