Astronomy & Astrophysics

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$\begin{figure} \par\includegraphics[width=8cm,height=8.2cm,clip]{3462fig1.eps} \end{figure}$ Figure 1: Einstein time histogram for differents amounts of blending. The curves give the relative number of short time events (below 66 days), binned in one-day time intervals. The curves are computed assuming a Poisson law with different values of $\bar n$ corresponding to different fractions of unblended stars (f).
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In the text

$\begin{figure} \par\includegraphics[width=7.5cm,height=8cm,clip]{3462fig2.eps} \end{figure}$ Figure 2: Ratio $\tau / \tau _{{\rm obs}}$ as a function of the unblended source fraction for different values of the LF cutoff. Standard values are $V_{{\rm inf}}=22$ and $V_{{\rm sup}}=16$ and these values are assumed except when indicated by the legend. Triangles and circles are computed using the same LF as the continuous line, but with model 2 and model 3 (see text).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,height=8.2cm,clip]{3462fig1.eps} \end{figure}$	Figure 1: Einstein time histogram for differents amounts of blending. The curves give the relative number of short time events (below 66 days), binned in one-day time intervals. The curves are computed assuming a Poisson law with different values of $\bar n$ corresponding to different fractions of unblended stars (f).
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.5cm,height=8cm,clip]{3462fig2.eps} \end{figure}$	Figure 2: Ratio $\tau / \tau _{{\rm obs}}$ as a function of the unblended source fraction for different values of the LF cutoff. Standard values are $V_{{\rm inf}}=22$ and $V_{{\rm sup}}=16$ and these values are assumed except when indicated by the legend. Triangles and circles are computed using the same LF as the continuous line, but with model 2 and model 3 (see text).
Open with DEXTER