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$\begin{figure} \par\includegraphics[angle=270,width=11cm,clip]{2wav.ps} \end{figure}$ Figure 1: Wavelengths for the Ca II $\lambda$ 8662-line vs. those of the $\lambda$ 8498-line. The open star is the laboratory position (NIST). The sun symbol marks the photospheric wavelengths. Stars showing the ⁴⁸Ca anomaly are in the upper-right portion of the diagram. There are two points (filled stars) for HD 101065. The large square is for HD 27411 and HD 187474 whose points overlap. The two halo stars, HD 140283 and HD 122563 are not plotted because the $\lambda$ 8662 line was not available. The sunspot was also not plotted because of the complexity of the $\lambda$ 8662 profile.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{fig2.ps} \end{figure}$ Figure 2: Spectra of 10 stars in the region of Ca II $\lambda$ 8498. Spectra have been displaced upward for purposes of illustration by amounts given in the text. The upper 7 stars are all magnetic stars. HD 27411 is an Am. HD 140283 is a well-studied subdwarf. The thin vertical lines are at $\lambda$ 8498.06 and 8498.20.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{fig2.ps} \end{figure}$	Figure 2: Spectra of 10 stars in the region of Ca II $\lambda$ 8498. Spectra have been displaced upward for purposes of illustration by amounts given in the text. The upper 7 stars are all magnetic stars. HD 27411 is an Am. HD 140283 is a well-studied subdwarf. The thin vertical lines are at $\lambda$ 8498.06 and 8498.20.
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