All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4294F1.ps} \end{figure}$ Figure 1: Hipparcos $H_{\rm P}$ and Tycho $V_{\rm T}, B_{\rm T}, (B-V)_{\rm T}$ lightcurves of V781 Tau folded onto the period P = 0.34490857 days. Radial velocity measurements in the GAIA spectral interval from Table 3 are given on the top, with "+'' signs marking blended spectral lines that were not used for modeling. The curves represent the solution given in Table 4.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4294F2.ps} \end{figure}$ Figure 2: Hipparcos $H_{\rm P}$ and Tycho $V_{\rm T}, B_{\rm T}, (B-V)_{\rm T}$ lightcurves of UV Leo folded onto the period P = 0.600086 days. Radial velocity measurements in the GAIA spectral interval from Table 3 are given on the top, with "+'' signs marking measurements around primary eclipse that were not considered in modeling. The curves represent the solution given in Table 4.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4294F3.ps} \end{figure}$ Figure 3: Hipparcos $H_{\rm P}$ and Tycho $V_{\rm T}, B_{\rm T}, (B-V)_{\rm T}$ lightcurves of GK Dra folded onto the period P = 9.9742 days. Radial velocity measurements in the GAIA spectral interval from Table 3 are given on the top. The curves represent the solution given in Table 4.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4294F1.ps} \end{figure}$	Figure 1: Hipparcos $H_{\rm P}$ and Tycho $V_{\rm T}, B_{\rm T}, (B-V)_{\rm T}$ lightcurves of V781 Tau folded onto the period P = 0.34490857 days. Radial velocity measurements in the GAIA spectral interval from Table 3 are given on the top, with "+'' signs marking blended spectral lines that were not used for modeling. The curves represent the solution given in Table 4.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4294F2.ps} \end{figure}$	Figure 2: Hipparcos $H_{\rm P}$ and Tycho $V_{\rm T}, B_{\rm T}, (B-V)_{\rm T}$ lightcurves of UV Leo folded onto the period P = 0.600086 days. Radial velocity measurements in the GAIA spectral interval from Table 3 are given on the top, with "+'' signs marking measurements around primary eclipse that were not considered in modeling. The curves represent the solution given in Table 4.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{H4294F3.ps} \end{figure}$	Figure 3: Hipparcos $H_{\rm P}$ and Tycho $V_{\rm T}, B_{\rm T}, (B-V)_{\rm T}$ lightcurves of GK Dra folded onto the period P = 9.9742 days. Radial velocity measurements in the GAIA spectral interval from Table 3 are given on the top. The curves represent the solution given in Table 4.
Open with DEXTER