All Figures

$\begin{figure} \par\includegraphics[width=87mm,clip]{G1133_f1.eps}\end{figure}$ Figure 1: Spectra of comet C/2001 Q4 at 3.7 AU (top) and 0.98 AU showing part of the R branch of the CN $\rm B-X$ (0, 0) band. The corresponding quantum numbers are indicated at the top. The major differences are related to the heliocentric distance and show up in the excitation of lines of higher quantum number when closer to the Sun. The intensity scale is relative only.
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In the text

$\begin{figure} \par\includegraphics[width=80mm,clip]{G1133_f2.eps} \end{figure}$ Figure 2: Nitrogen and carbon isotopic ratios at various heliocentricdistances.
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In the text

$\begin{figure} \par\includegraphics[width=87mm,clip]{G1133_f1.eps}\end{figure}$	Figure 1: Spectra of comet C/2001 Q4 at 3.7 AU (top) and 0.98 AU showing part of the R branch of the CN $\rm B-X$ (0, 0) band. The corresponding quantum numbers are indicated at the top. The major differences are related to the heliocentric distance and show up in the excitation of lines of higher quantum number when closer to the Sun. The intensity scale is relative only.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=80mm,clip]{G1133_f2.eps} \end{figure}$	Figure 2: Nitrogen and carbon isotopic ratios at various heliocentricdistances.
Open with DEXTER