$\begin{figure} \par\includegraphics[width=8cm,clip]{h4327f1.eps} \end{figure}$ Figure 1: Spectral features in the "late" Ae/Be Herbig star HD 31648. Note the sharp feature in the center of DIB 5780 (it is a stellar Fe II line) and the extremely weak Ca II H line.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4327f2.eps} \end{figure}$ Figure 2: Features seen in the spectrum of HD 36917. Note the weak emission in Na I (D2). Red-shifting is a common characteristic of DIBs, seen in the spectra of the Orion nebula stars.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4327f4.eps} \end{figure}$ Figure 4: Features seen in the spectrum of HD 179218. The DIB 6284 profiles contain sharp remnants of unremoved telluric lines.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{h4327f5.eps} \end{figure}$ Figure 5: Complex spectral features of HD 190073. The central part of DIB 5780 is blended with the Fe II line. The blue shifted double components seen in the Ca II lines were already reported by Merrill (1950). DIB 6284 is contaminated by sharp telluric lines.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{h4327f6.eps} \end{figure}$ Figure 6: Broad emission is seen in the atomic lines of HD 250550. Note very weak "narrow" DIBs (6614 and 5797) in contrast to the clear DIB 5780.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{h4327f7.eps} \end{figure}$ Figure 7: The comparison of the general average spectrum of all the considered stars (except HD 36917) with a spectrum of a well-known $\sigma$ type object: HD 144217. In both spectra the 5797 feature is normalized to unity.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4327f1.eps} \end{figure}$	Figure 1: Spectral features in the "late" Ae/Be Herbig star HD 31648. Note the sharp feature in the center of DIB 5780 (it is a stellar Fe II line) and the extremely weak Ca II H line.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4327f2.eps} \end{figure}$	Figure 2: Features seen in the spectrum of HD 36917. Note the weak emission in Na I (D2). Red-shifting is a common characteristic of DIBs, seen in the spectra of the Orion nebula stars.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{h4327f3.eps} \end{figure}$	Figure 3: Spectral features seen in the spectrum of HD 50138.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{h4327f4.eps} \end{figure}$	Figure 4: Features seen in the spectrum of HD 179218. The DIB 6284 profiles contain sharp remnants of unremoved telluric lines.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{h4327f5.eps} \end{figure}$	Figure 5: Complex spectral features of HD 190073. The central part of DIB 5780 is blended with the Fe II line. The blue shifted double components seen in the Ca II lines were already reported by Merrill (1950). DIB 6284 is contaminated by sharp telluric lines.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{h4327f6.eps} \end{figure}$	Figure 6: Broad emission is seen in the atomic lines of HD 250550. Note very weak "narrow" DIBs (6614 and 5797) in contrast to the clear DIB 5780.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.9cm,clip]{h4327f7.eps} \end{figure}$	Figure 7: The comparison of the general average spectrum of all the considered stars (except HD 36917) with a spectrum of a well-known $\sigma$ type object: HD 144217. In both spectra the 5797 feature is normalized to unity.
Open with DEXTER