EDP Sciences
Free Access
Issue
A&A
Volume 508, Number 3, December IV 2009
Page(s) 1313 - 1330
Section Galactic structure, stellar clusters, and populations
DOI https://doi.org/10.1051/0004-6361/200913327
Published online 04 November 2009

Online Material

\begin{figure}
{\hspace{1cm} \includegraphics[width=7.5cm,height=9cm]{13327f21.eps} }
\end{figure} Figure 21:

The flare event observed on Star #11 (2MASS J05352550-0545448 = NR Ori) on December 10th, 2006 at 3:30 UT in the I band (upper panel). The simultaneous J light curve (bottom panel) does not show any clear variation.

Open with DEXTER

\begin{figure}
\par\mbox{\includegraphics[width=5.5cm]{3327f22a.eps} \includegra...
...5.5cm]{3327f22b.eps} \includegraphics[width=5.5cm]{3327f22c.eps} }\end{figure} Figure 22:

Light curves in the R, I, and J band of the five variable stars for which we could not find any reliable period.

Open with DEXTER

\begin{figure}
\par\mbox{\includegraphics[width=5.9cm,clip]{3327f23a.eps} \inclu...
...]{3327f23b.eps} \includegraphics[width=5.9cm,clip]{3327f23c.eps} }\end{figure} Figure 23:

Hectochelle spectra in the H$\alpha $ region of our targets (black lines) with the best templates superimposed (thin red lines). The H$\alpha $ emission has been cut in order to display the photospheric absorption lines. The Id number is marked in the top-left corner of each box.

Open with DEXTER

\begin{figure}\par\mbox{\includegraphics[width=5.5cm]{3327f24a.eps} \includegrap...
....5cm]{3327f24b.eps} \includegraphics[width=5.5cm]{3327f24c.eps} }
\end{figure} Figure 24:

Hectochelle spectra in the Mg I b region of our targets (black lines) with the best templates superimposed (thin red lines). The Id number is marked in the top-left corner of each box.

Open with DEXTER

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