Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=8cm,clip]{3219fig2.eps} \end{figure}$ Figure 1: The observed spectrum of CH Cyg in the region of well-known Ca index. Also shown is the spectrum of the Sun (Wallace et al. 1996).
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In the text

$\begin{figure} \par\includegraphics[width=12cm,clip]{3219fig3.eps}\end{figure}$ Figure 3: The observed (thick line) and synthetic spectra calculated using final abundances of the symbiotic star CH Cyg in the spectral region from 1.582 to 1.586 $\mu$ m are shown on the top. The synthesized CN, OH, ¹²CO, and atomic components are presented separately. Atomic lines are identified by ticks.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{3219fig4.eps} \end{figure}$ Figure 4: The observed spectra (thick solid an dashed) of CH Cyg in the region of (2-0) ¹²C¹⁶O band head for two different phases of symbiotic activity. Also shown is the calculated spectrum (thin solid) using the final atmospheric parameters and abundances.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{3219fig2.eps} \end{figure}$	Figure 1: The observed spectrum of CH Cyg in the region of well-known Ca index. Also shown is the spectrum of the Sun (Wallace et al. 1996).
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$\begin{figure} \par\includegraphics[width=8cm,clip]{3219fig1.eps} \end{figure}$	Figure 2: Same as Fig. 1, but around the Na index.
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$\begin{figure} \par\includegraphics[width=12cm,clip]{3219fig3.eps}\end{figure}$	Figure 3: The observed (thick line) and synthetic spectra calculated using final abundances of the symbiotic star CH Cyg in the spectral region from 1.582 to 1.586 $\mu$ m are shown on the top. The synthesized CN, OH, ¹²CO, and atomic components are presented separately. Atomic lines are identified by ticks.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{3219fig4.eps} \end{figure}$	Figure 4: The observed spectra (thick solid an dashed) of CH Cyg in the region of (2-0) ¹²C¹⁶O band head for two different phases of symbiotic activity. Also shown is the calculated spectrum (thin solid) using the final atmospheric parameters and abundances.
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