All Figures

$\begin{figure} \par\includegraphics[width=16.3cm,clip]{5450fig1.eps}\end{figure}$ Figure 1: Photometric data collected in 2000/01 in Strömgren v and y with the APT (filled squares) and at the observatory OSN (open triangles). $\Delta v$ and $\Delta y$ are the observed magnitude differences (variable minus comparison star). The calculated fit (including all detected frequencies) is shown as a solid curve. The lightcurves from 2001/02 and 2002/03 are not shown in this paper.
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In the text

$\begin{figure} \par\includegraphics[width=14.9cm,clip]{5450fig2.eps}\end{figure}$ Figure 2: Power spectra of 44 Tau, showing the Strömgren v data from 2000 to 2003 in the 5 to 35 cd^-1 region, before and after prewhitening. The daily and the annual spectral windows are presented. In the lower panel 28 frequencies were prewhitened.
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In the text

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{5450fig3.eps}\end{figure}$ Figure 3: In this figure the Strömgren y amplitudes of the seven dominant frequencies, also using previous Johnson V data from Paper I and Park (1993) are shown. One can see a clear amplitude variability of 7.0060 cd^-1 and 9.5613 cd^-1. A variation of 9.1175 cd^-1 is possible.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{5450fig4.eps}\end{figure}$ Figure 4: The frequency spectrum of 44 Tau without the identified radial modes f₁ and f₅. One can see that an unambiguous pattern of multiplets due to rotation is not present.
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In the text

$\begin{figure} \par\includegraphics[width=14.9cm,clip]{5450fig2.eps}\end{figure}$	Figure 2: Power spectra of 44 Tau, showing the Strömgren v data from 2000 to 2003 in the 5 to 35 cd^-1 region, before and after prewhitening. The daily and the annual spectral windows are presented. In the lower panel 28 frequencies were prewhitened.
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$\begin{figure} \par\includegraphics[width=8.1cm,clip]{5450fig3.eps}\end{figure}$	Figure 3: In this figure the Strömgren y amplitudes of the seven dominant frequencies, also using previous Johnson V data from Paper I and Park (1993) are shown. One can see a clear amplitude variability of 7.0060 cd^-1 and 9.5613 cd^-1. A variation of 9.1175 cd^-1 is possible.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{5450fig4.eps}\end{figure}$	Figure 4: The frequency spectrum of 44 Tau without the identified radial modes f₁ and f₅. One can see that an unambiguous pattern of multiplets due to rotation is not present.
Open with DEXTER