$\begin{figure} \par\includegraphics[width=8.8cm,clip]{BV_det.ps} \end{figure}$ Figure 2: Color-magnitude diagram (B-V vs. M_V) for all X-ray detected stars listed in the NEXXUS data base.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{fig1a.ps} \end{figure}$ Figure 3: $L_{\rm X}$ vs. distance for the F/G star sample; note the complete sampling out to 12 pc.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{fig1b.ps} \end{figure}$ Figure 4: $L_{\rm X}$ vs. distance for the K star sample; note the complete sampling out to 8 pc; the two upper limits come from survey data.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{MvLx.ps} \end{figure}$ Figure 6: X-ray luminosity vs. absolute magnitude M_V for the nearby main-sequence stars; plusses denote F/G-type stars, asterisks K-type stars and crosses M-type stars. Note the absence of solar-like stars with X-ray luminosities of 10²⁶ erg/s and below.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{MvFx.ps} \end{figure}$ Figure 7: Mean X-ray surface flux vs. absolute magnitude M_V for the nearby main-sequence stars; plusses denote F/G-type stars, asterisks K-type stars and crosses M-type stars. Note the lower limit of about 10⁴ erg/cm²/s of observed X-ray surface flux.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{cumulative.ps} \end{figure}$ Figure 8: Cumulative distribution function of the mean X-ray surface fluxes for F/G-type stars (stepped curve), K-type stars (dotted stepped curve) and M-type stars (dashed stepped curve). Note the close resemblance of the curves with indistinguishable mean and minimum.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{PtoS.ps} \end{figure}$ Figure 9: Comparison of X-ray count rates for sample stars detected both in the all-sky survey and the PSPC pointing program; dashed lines indicate a factor 2 variation from unity and stars with large deviations from regression line are identified.
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In the text

$\begin{figure} \par\includegraphics[width=8.7cm,clip]{PtoF.ps} %\end{figure}$ Figure 10: Comparison of X-ray count rates for all NEXXUS stars detected in the PSPC pointing program with and without boron filter; stars with large deviations from regression line are identified.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{PtoH.ps} % \par \end{figure}$ Figure 11: Comparison of X-ray count rates for all NEXXUS stars detected both in the PSPC and HRI pointing program; stars with large deviations from regression line are identified.
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{Gl559ab1.ps} % \par \end{figure}$ Figure 12: X-ray light curve for $\alpha$ Cen A/B (Gl 559AB) in February 1996; asterisks denote measurements for $\alpha$ Cen B, plusses measurements for $\alpha$ Cen A.
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In the text

$\begin{figure} \par\includegraphics[width=8.3cm,clip]{Gl559ab2.ps} %\end{figure}$ Figure 13: X-ray light curve for $\alpha$ Cen A/B (Gl 559AB) in August 1996; asterisks denote measurements for $\alpha$ Cen B, plusses measurements for $\alpha$ Cen A.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{BV_all.ps} \end{figure}$	Figure 1: Color-magnitude diagram (B-V vs. M_V) for all stars contained in CNS4 catalog.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{BV_det.ps} \end{figure}$	Figure 2: Color-magnitude diagram (B-V vs. M_V) for all X-ray detected stars listed in the NEXXUS data base.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{fig1a.ps} \end{figure}$	Figure 3: $L_{\rm X}$ vs. distance for the F/G star sample; note the complete sampling out to 12 pc.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{fig1b.ps} \end{figure}$	Figure 4: $L_{\rm X}$ vs. distance for the K star sample; note the complete sampling out to 8 pc; the two upper limits come from survey data.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{fig1c.ps} \end{figure}$	Figure 5: $L_{\rm X}$ vs. distance for the M star sample.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{MvLx.ps} \end{figure}$	Figure 6: X-ray luminosity vs. absolute magnitude M_V for the nearby main-sequence stars; plusses denote F/G-type stars, asterisks K-type stars and crosses M-type stars. Note the absence of solar-like stars with X-ray luminosities of 10²⁶ erg/s and below.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{MvFx.ps} \end{figure}$	Figure 7: Mean X-ray surface flux vs. absolute magnitude M_V for the nearby main-sequence stars; plusses denote F/G-type stars, asterisks K-type stars and crosses M-type stars. Note the lower limit of about 10⁴ erg/cm²/s of observed X-ray surface flux.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{cumulative.ps} \end{figure}$	Figure 8: Cumulative distribution function of the mean X-ray surface fluxes for F/G-type stars (stepped curve), K-type stars (dotted stepped curve) and M-type stars (dashed stepped curve). Note the close resemblance of the curves with indistinguishable mean and minimum.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{PtoS.ps} \end{figure}$	Figure 9: Comparison of X-ray count rates for sample stars detected both in the all-sky survey and the PSPC pointing program; dashed lines indicate a factor 2 variation from unity and stars with large deviations from regression line are identified.
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$\begin{figure} \par\includegraphics[width=8.7cm,clip]{PtoF.ps} %\end{figure}$	Figure 10: Comparison of X-ray count rates for all NEXXUS stars detected in the PSPC pointing program with and without boron filter; stars with large deviations from regression line are identified.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{PtoH.ps} % \par \end{figure}$	Figure 11: Comparison of X-ray count rates for all NEXXUS stars detected both in the PSPC and HRI pointing program; stars with large deviations from regression line are identified.
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$\begin{figure} \par\includegraphics[width=8.3cm,clip]{Gl559ab1.ps} % \par \end{figure}$	Figure 12: X-ray light curve for $\alpha$ Cen A/B (Gl 559AB) in February 1996; asterisks denote measurements for $\alpha$ Cen B, plusses measurements for $\alpha$ Cen A.
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$\begin{figure} \par\includegraphics[width=8.3cm,clip]{Gl559ab2.ps} %\end{figure}$	Figure 13: X-ray light curve for $\alpha$ Cen A/B (Gl 559AB) in August 1996; asterisks denote measurements for $\alpha$ Cen B, plusses measurements for $\alpha$ Cen A.
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$\begin{figure} \par\includegraphics[width=8.14cm,clip]{Gl86.ps} \end{figure}$	Figure 14: X-ray light curve for Gl 86 in May/June 1993.
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