All Figures

$\begin{figure} \par\includegraphics[width=400pt]{12co_br.ps}\end{figure}$ Figure 1: ¹²CO 3-2 lines of selected sources in Lupus, with off-positions 30'' south and east of source.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=250pt]{c18o_final.ps}\end{figure}$ Figure 2: C¹⁸O lines toward selected sources in Lupus.
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In the text

$\begin{figure} \par\includegraphics[width=230pt]{imlup_final.ps}\end{figure}$ Figure 3: ¹²CO 3-2, ¹³CO 3-2, and C¹⁸O 2-1 spectra observed toward IM Lup (Sz 82) shifted by +4, +2, and 0 K, respectively.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=230pt]{bestest_fit.ps}\end{figure}$ Figure 4: Comparison of the observed ¹²CO J=3-2 line toward IM Lup with the best-model fit with a disk of $i=20^\circ$ , R=600 AU.
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In the text

$\begin{figure} \par\includegraphics[width=230pt]{gqlup_new_cor.eps}\end{figure}$ Figure 5: ¹²CO 3-2, ¹³CO 3-2, and C¹⁸O 2-1 lines toward GQ Lup, shifted by +4, +2, and 0 K, respectively.
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In the text

$\begin{figure}\par\mbox{\includegraphics[width=140pt]{online/12co/hmlup.ps} \inc... .../sz123.ps} \includegraphics[width=140pt]{online/12co/v908sco.ps} } \end{figure}$ Figure 6: ¹²CO 3-2 lines of selected sources in Lupus, with off-positions 30'' south and east of source.
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In the text