$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152S_D.eps} \end{figure}$ Figure 7: Spectral slope plotted versus diameter for Cybele asteroids. Results from the present study have been marked by asterisks, values from the literature are represented by open circles.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152fig_a.eps} \end{figure}$	Figure 1: Spectra for the asteroids (420) Bertholda, (522) Helga, (536) Merapi and (643) Scheherezade. The spectra have been shifted vertically for clarity.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152fig_b.eps} \end{figure}$	Figure 2: Spectra for the asteroids (721) Tabora, (1004) Belopolskya, (1266) Tone and (1574) Meyer.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152fig_c.eps} \end{figure}$	Figure 3: Spectra for the asteroids (2634) James Bradley, (3015) Candy, (3095) Omarkhayyam and (3622) Ilinsky.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152fig_d.eps} \end{figure}$	Figure 4: Spectra for the asteroids (3675) Kemstach, (4003) Schumann, (4158) Santini and (4973) Showa.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152fig_e.eps} \end{figure}$	Figure 5: Spectra for the asteroids (5780) Lafontaine and (5833) Peterson.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152fig_f.eps} \end{figure}$	Figure 6: Spectrum of the asteroid (4014) Heizman.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1152S_D.eps} \end{figure}$	Figure 7: Spectral slope plotted versus diameter for Cybele asteroids. Results from the present study have been marked by asterisks, values from the literature are represented by open circles.
Open with DEXTER