Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{Fb174F1.ps} \end{figure}$ Figure 1: VLT/NACO AO imaging of the unresolved triple system TY CrA and the fourth stellar component candidate detected at $0.3\hbox {$^{\prime \prime }$ }$ at $1.257~\mu$ m and $2.166~\mu$ m. North is up and east is left.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Fb174F2.ps} \end{figure}$ Figure 2: Evolutionary tracks of Baraffe et al. (1998) with the location of the fourth stellar component candidate to TY CrA based on photometry and assuming an age between 3.2 and 4 Myr for 3 hypothesis of distance: 161 pc, 136 pc and 117 pc (from left to right).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.8cm,clip]{Fb174F1.ps} \end{figure}$	Figure 1: VLT/NACO AO imaging of the unresolved triple system TY CrA and the fourth stellar component candidate detected at $0.3\hbox {$^{\prime \prime }$ }$ at $1.257~\mu$ m and $2.166~\mu$ m. North is up and east is left.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{Fb174F2.ps} \end{figure}$	Figure 2: Evolutionary tracks of Baraffe et al. (1998) with the location of the fourth stellar component candidate to TY CrA based on photometry and assuming an age between 3.2 and 4 Myr for 3 hypothesis of distance: 161 pc, 136 pc and 117 pc (from left to right).
Open with DEXTER