All Figures

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3765f1.ps} \end{figure}$ Figure 1: The B and V light curves of V497 Cep, based on Ege University observations.
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,clip]{3765f2.ps} \end{figure}$ Figure 2: Selected He I 6678 profiles of V497 Cep. The profiles are identified by phase according to ephemeris (1). Longer tick marks on the flux scale are separated for 0.2 of relative flux units.
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In the text

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{3765f3.ps} \end{figure}$ Figure 3: Selected H $\alpha$ 6563 profiles of V497 Cep. The profiles are identified by phase according to ephemeris (1). Longer tick marks on the flux scale are separated for 0.2 of relative flux units.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3765f4a.eps}\vspace*{3mm} \includegraphics[width=8.8cm,clip]{3765f4b.eps} \end{figure}$ Figure 4: A comparison of radial-velocity curves of the primary and secondary measured directly in SPEFO (upper panel) and based on KOREL disentangling (bottom panel). Filled symbols refer to the primary and the Crimean spectra are shown by circles, and the DAO spectra by triangles. The final ephemeris (2) was used.
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{3765f5a.eps}\par\includegraphics[width=8.7cm,clip]{3765f5b.eps} \end{figure}$ Figure 5: He I 6678 line profiles of primary and secondary disentangled via KOREL (solid lines) are compared with synthetic LTE line profiles shifted for the systemic velocity of -19 km s^-1 and rotationally broadened to projected rotational velocities of 132 and 104 km s^-1, for the primary and secondary, respectively, which correspond to spin-orbit synchronization. Wavelengths are in Å and the disentangled profiles from KOREL were normalized using the luminosity ratio from the V light-curve solution - see the text for details.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{3765f6.ps} \end{figure}$ Figure 6: A comparison of the observed (dots) and computed (solid line) B light curves of V497 Cep.
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{3765f7a.eps}\par\includegraphics[width=8.7cm,clip]{3765f7b.eps} \end{figure}$ Figure 7: The positions of the stellar components of the eclipsing, double-lined binary V497 Cep in the a) log $L/L_\odot$ - log $T_{\rm eff}$ and b) log $R/R_\odot$ - log $T_{\rm eff}$ diagrams. Masses of corresponding evolutionary models are indicated near the corresponding points with both, zero-age (ZAMS) and terminal-age (TAMS) main sequence locations.
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3765f1.ps} \end{figure}$	Figure 1: The B and V light curves of V497 Cep, based on Ege University observations.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.4cm,clip]{3765f2.ps} \end{figure}$	Figure 2: Selected He I 6678 profiles of V497 Cep. The profiles are identified by phase according to ephemeris (1). Longer tick marks on the flux scale are separated for 0.2 of relative flux units.
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$\begin{figure} \par\includegraphics[width=7.9cm,clip]{3765f3.ps} \end{figure}$	Figure 3: Selected H $\alpha$ 6563 profiles of V497 Cep. The profiles are identified by phase according to ephemeris (1). Longer tick marks on the flux scale are separated for 0.2 of relative flux units.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{3765f4a.eps}\vspace*{3mm} \includegraphics[width=8.8cm,clip]{3765f4b.eps} \end{figure}$	Figure 4: A comparison of radial-velocity curves of the primary and secondary measured directly in SPEFO (upper panel) and based on KOREL disentangling (bottom panel). Filled symbols refer to the primary and the Crimean spectra are shown by circles, and the DAO spectra by triangles. The final ephemeris (2) was used.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{3765f6.ps} \end{figure}$	Figure 6: A comparison of the observed (dots) and computed (solid line) B light curves of V497 Cep.
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$\begin{figure} \par\includegraphics[width=8.7cm,clip]{3765f7a.eps}\par\includegraphics[width=8.7cm,clip]{3765f7b.eps} \end{figure}$	Figure 7: The positions of the stellar components of the eclipsing, double-lined binary V497 Cep in the a) log $L/L_\odot$ - log $T_{\rm eff}$ and b) log $R/R_\odot$ - log $T_{\rm eff}$ diagrams. Masses of corresponding evolutionary models are indicated near the corresponding points with both, zero-age (ZAMS) and terminal-age (TAMS) main sequence locations.
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