$\begin{figure} \par\includegraphics[width=8.4cm,clip]{5967fig1.eps} \end{figure}$ Figure 1: The 90 $\hbox {$^{\prime \prime }$ }\times 90\hbox {$^{\prime \prime }$ }$ extraction from the summarized image observed through V and R filters. North, East, and sunward directions are indicated. The vertical line across the comet marks the position of the slit in the spectroscopic mode.
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In the text

$\begin{figure} \par\includegraphics[width=15cm,clip]{5967fig2.eps} \end{figure}$ Figure 2: Observed spectrum and flux ratio plot comet/Sun for C/2002 VQ94 (LINEAR). Assigned molecular emissions are marked. Filled features at the bottom of the plot show the CO⁺ spectrum calculated under the Boltzmann approximation (Kim 1994, 1998).
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In the text

$\begin{figure} \par\includegraphics[width=15cm,clip]{5967fig3.eps} \end{figure}$ Figure 3: Spectrum of comet C/2002 VQ94 (LINEAR) ( top) is displayed together with a part of the comet Humason (1962 VIII) spectrogram ( bottom) to compare available molecular emissions. The spectrogram of comet Humason is taken from Arpigny (1972). Identifications of principal features are indicated as well.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{5967fig1.eps} \end{figure}$	Figure 1: The 90 $\hbox {$^{\prime \prime }$ }\times 90\hbox {$^{\prime \prime }$ }$ extraction from the summarized image observed through V and R filters. North, East, and sunward directions are indicated. The vertical line across the comet marks the position of the slit in the spectroscopic mode.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15cm,clip]{5967fig2.eps} \end{figure}$	Figure 2: Observed spectrum and flux ratio plot comet/Sun for C/2002 VQ94 (LINEAR). Assigned molecular emissions are marked. Filled features at the bottom of the plot show the CO⁺ spectrum calculated under the Boltzmann approximation (Kim 1994, 1998).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15cm,clip]{5967fig3.eps} \end{figure}$	Figure 3: Spectrum of comet C/2002 VQ94 (LINEAR) ( top) is displayed together with a part of the comet Humason (1962 VIII) spectrogram ( bottom) to compare available molecular emissions. The spectrogram of comet Humason is taken from Arpigny (1972). Identifications of principal features are indicated as well.
Open with DEXTER