$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{97678.eps} \end{figure}$ Figure 1: Section of the millimeter wave spectrum of CH₃OH showing asymmetry splitting in the v_t = 0, J_k = 21₆-22₅ transitions of A symmetry. Each line appears approximately as a second derivative of a Gaussian because of the 2f-modulation employed to reduce noise and baseline effects.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{96747.eps} \end{figure}$ Figure 2: Section of the millimeter wave spectrum of CH₃OH showing part of the v_t = 0, J = 2-1 a-type transitions ( $\Delta K = 0$ ) which are observable in dark clouds. The k values and the symmetry are indicated. See also caption to Fig. 1.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{97678.eps} \end{figure}$	Figure 1: Section of the millimeter wave spectrum of CH₃OH showing asymmetry splitting in the v_t = 0, J_k = 21₆-22₅ transitions of A symmetry. Each line appears approximately as a second derivative of a Gaussian because of the 2f-modulation employed to reduce noise and baseline effects.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{96747.eps} \end{figure}$	Figure 2: Section of the millimeter wave spectrum of CH₃OH showing part of the v_t = 0, J = 2-1 a-type transitions ( $\Delta K = 0$ ) which are observable in dark clouds. The k values and the symmetry are indicated. See also caption to Fig. 1.
Open with DEXTER