All Figures

$\begin{figure} \par\includegraphics{11395f1.eps} \end{figure}$ Figure 1: Differences of the geocentric right ascensions of perturbed bodies caused by (4) Vesta ( left) and mutual distances between perturbed asteroids and (4) Vesta ( right). Differences of the geocentric right ascensions of perturbed bodies calculated at the instances of available sets of observations are denoted by asterisks. Pairs of plots from the top to the bottom correspond to close encounters with: (3057) Malaren, (5205) 1988CU7, (8331) Dawkins and (21225) 1995GQ1, respectively.
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In the text

$\begin{figure} \par\includegraphics{11395f2.eps} \end{figure}$ Figure 2: Differences of the geocentric right ascensions of (17) Thetis (curve on lowest position), (67) Asia (curve on medium position) and (197) Arete (curve on highest position) caused by (4) Vesta.
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In the text

$\begin{figure} \par\includegraphics{11395f2.eps} \end{figure}$	Figure 2: Differences of the geocentric right ascensions of (17) Thetis (curve on lowest position), (67) Asia (curve on medium position) and (197) Arete (curve on highest position) caused by (4) Vesta.
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