All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{0833fig1.eps}\end{figure}$ Figure 1: A section of the May 6 spectrum of the OH (1, 1) band in comet C/2002 T7. Black: observed spectrum; blue: synthetic emission spectrum of ¹⁶OH fitted to the observed one (the extended wings of the ¹⁶OH lines are not modelled here; on the other hand, in this and all three other figures, the presence of prompt emission is taken into account); red: synthetic fluorescence spectrum of ¹⁸OH with the typical ratio ¹⁶OH/¹⁸OH = 500. The position of the ¹⁸OH lines at 3134.315 Å and 3137.459 Å is indicated.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0833fig2.eps}\end{figure}$ Figure 2: Co-addition of the ¹⁸OH lines at $\lambda = 3134.315$ Å, 3137.459 Å and 3142.203 Å from the May 6 spectrum after proper wavelength shifts. Co-added ¹⁸OH is shifted to $\lambda =0$ while ¹⁶OH appears at $\lambda \simeq 0.3$ . Black: observed spectrum; red: synthetic combined spectrum of ¹⁶OH, ¹⁸OH with ¹⁶OH/¹⁸OH = 410, and an empirical fit to the OH extended wings.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0833fig3.eps}\end{figure}$ Figure 3: Co-addition of 27 OD lines from the May 6 spectrum after proper wavelength shifts. Co-added OD is shifted to $\lambda =0$ . Black: observed spectrum; red: synthetic combined spectrum of OH, OD with OD/OH = $4\times 10^{-4}$ , and an empirical fit to the OH extended wings.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0833fig4.eps}\end{figure}$ Figure 4: Same as Fig. 3 for the May 26 spectrum.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0833fig3.eps}\end{figure}$	Figure 3: Co-addition of 27 OD lines from the May 6 spectrum after proper wavelength shifts. Co-added OD is shifted to $\lambda =0$ . Black: observed spectrum; red: synthetic combined spectrum of OH, OD with OD/OH = $4\times 10^{-4}$ , and an empirical fit to the OH extended wings.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{0833fig4.eps}\end{figure}$	Figure 4: Same as Fig. 3 for the May 26 spectrum.
Open with DEXTER