All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=6cm,clip]{9797fig1.ps} \end{figure}$ Figure 1: Distribution of NLTT proper motions. Dots show the NLTT stars with $\mu >0.18$ arcsec/yr and proper motion components of less than $\pm$ 1 arcsec/yr. The two large circles show proper motion limits of 0.850 and 0.865 arcsec/yr. Small filled circles mark the NLTT stars falling between these proper motion limits. The straight line shows the position angles of the proper motions of SSSPM 1930/SSSPM 2003.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{9797fig2.ps} % \end{figure}$ Figure 2: Distribution of all NLTT stars with $\mu >0.18$ arcsec/yr on the sky. Small filled circles mark the NLTT stars with proper motions between 0.850 and 0.865 arcsec/yr. The two filled squares mark the positions of SSSPM 1930 and SSSPM 2003.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{9797fig3.ps} % \end{figure}$ Figure 3: Low-resolution classification spectra of SSSPM 1930, SSSPM 2003 and some comparison objects. The ESO NTT/EMMI spectrum of SSSPM 1930 is from Scholz et al. (2004), the Keck/LRIS spectrum of LHS 377 was taken from Neill Reid's Web page (http://dept.physics.upenn.edu/~inr/ultracool.html). The ESO 3.6 m/EFOSC2 spectrum of SSSPM 2003 is shown together with ESO VLT/FORS1 spectra of two comparison objects from Lodieu et al. (2005): LP 859-1 and LHS 3141B. All spectra are flux-calibrated and normalised at 7500 Å.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{9797fig4.ps} % \end{figure}$ Figure 4: UVW velocities of 35 682 CRVAD-2 stars (dots). Four stars with velocity components within 50 km s^-1 (squares) of the mean velocity of SSSPM 1930 and SSSPM 2003 are marked (circles).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{9797fig2.ps} % \end{figure}$	Figure 2: Distribution of all NLTT stars with $\mu >0.18$ arcsec/yr on the sky. Small filled circles mark the NLTT stars with proper motions between 0.850 and 0.865 arcsec/yr. The two filled squares mark the positions of SSSPM 1930 and SSSPM 2003.
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$\begin{figure} \par\includegraphics[angle=-90,width=8cm,clip]{9797fig4.ps} % \end{figure}$	Figure 4: UVW velocities of 35 682 CRVAD-2 stars (dots). Four stars with velocity components within 50 km s^-1 (squares) of the mean velocity of SSSPM 1930 and SSSPM 2003 are marked (circles).
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