All Figures

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{FIG_1A_H3970.ps}\par\vspace*{2mm} \includegraphics[width=8.5cm,clip]{FIG_1B_H3970.ps} \end{figure}$ Figure 1: Spectral Energy Distribution of radio galaxies. The values of $\nu L_{\nu }$ are in erg s^-1.
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{FIG_2_H3970.ps} \end{figure}$ Figure 2: Core luminosities $L_{\nu {\rm X}}$ (erg s^-1 Hz^-1 at 1 keV) in the X-ray band of BL Lacs and radio galaxies (the latter ones indicated by empty squares) vs. the extended radio luminosity $L_{\nu {\rm r}, {\rm ext}}$ (erg s^-1 Hz^-1 at 1.4 GHz.). Filled triangles: LBL; crosses: HBL.
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{FIG_3_H3970.ps} \end{figure}$ Figure 3: Plot of the broad-band spectral indices $\alpha _{\rm ro}$ and $\alpha _{\rm rX}$ vs. $\alpha _{\rm oX}$ for our sample, including also the sources of Paper I (3C 288 is not included as it is found $\alpha _{\rm oX} > 0.34$ ). The regions occupied by LBL and HBL are from Fossati et al. (1998).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{FIG_4_H3970.ps} \end{figure}$ Figure 4: Left panels: Beaming tracks of $\alpha _{\rm ro}$ and $\alpha _{\rm rX}$ vs. $\alpha _{\rm oX}$ for 3C 272.1 for no absorption (solid lines) and 1.5 mag of extinction (dash-dotted lines) at optical wavelengths. It has been assumed for the spectral indices $\alpha _{\rm X}=1.3$ , $\alpha _{\rm r}=0$ , and $\alpha _{\rm o}= 0.5$ (leftwards tracks) and $\alpha _{\rm o}= 1.5$ (rightwards tracks). The shadowed regions limit the values of allowed $R_{\delta }$ deduced from the comparison of $L_{\nu {\rm X}}$ with $L_{\nu {\rm r}, {\rm ext}}$ (see Sect. 4). Right panels: Tracks of $L_{\nu {\rm r}}$ and $L_{\nu {\rm X}}$ vs. $L_{\nu {\rm o}}$ (erg s^-1 Hz^-1) for the same parameters (upper tracks: $\alpha _{\rm o}= 0.5$ , lower tracks: $\alpha _{\rm o}= 1.5$ ).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{FIG_5_H3970.ps} \end{figure}$ Figure 5: The same as Fig. 4 for 3C 66B, assuming $\alpha _{\rm X}=0.3$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{FIG_6_H3970.ps} \end{figure}$ Figure 6: The same as Fig. 4 for 3C 346, assuming $\alpha _{\rm X}=0.7$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{FIG_7_H3970.ps} \end{figure}$ Figure 7: The same as Fig. 4 for 3C 264, assuming $\alpha _{\rm X}=1.45$ .
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In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{FIG_1A_H3970.ps}\par\vspace*{2mm} \includegraphics[width=8.5cm,clip]{FIG_1B_H3970.ps} \end{figure}$	Figure 1: Spectral Energy Distribution of radio galaxies. The values of $\nu L_{\nu }$ are in erg s^-1.
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$\begin{figure} \par\includegraphics[width=8.3cm,clip]{FIG_2_H3970.ps} \end{figure}$	Figure 2: Core luminosities $L_{\nu {\rm X}}$ (erg s^-1 Hz^-1 at 1 keV) in the X-ray band of BL Lacs and radio galaxies (the latter ones indicated by empty squares) vs. the extended radio luminosity $L_{\nu {\rm r}, {\rm ext}}$ (erg s^-1 Hz^-1 at 1.4 GHz.). Filled triangles: LBL; crosses: HBL.
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$\begin{figure} \par\includegraphics[width=8.3cm,clip]{FIG_3_H3970.ps} \end{figure}$	Figure 3: Plot of the broad-band spectral indices $\alpha _{\rm ro}$ and $\alpha _{\rm rX}$ vs. $\alpha _{\rm oX}$ for our sample, including also the sources of Paper I (3C 288 is not included as it is found $\alpha _{\rm oX} > 0.34$ ). The regions occupied by LBL and HBL are from Fossati et al. (1998).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{FIG_5_H3970.ps} \end{figure}$	Figure 5: The same as Fig. 4 for 3C 66B, assuming $\alpha _{\rm X}=0.3$ .
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{FIG_6_H3970.ps} \end{figure}$	Figure 6: The same as Fig. 4 for 3C 346, assuming $\alpha _{\rm X}=0.7$ .
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{FIG_7_H3970.ps} \end{figure}$	Figure 7: The same as Fig. 4 for 3C 264, assuming $\alpha _{\rm X}=1.45$ .
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