EDP Sciences
Free Access
Issue
A&A
Volume 520, September-October 2010
Article Number A94
Number of page(s) 7
Section Galactic structure, stellar clusters, and populations
DOI https://doi.org/10.1051/0004-6361/201014799
Published online 08 October 2010

Online Material

\begin{figure}
\par\includegraphics[width=4.5cm]{14799f15.eps}\includegraphics[w...
...dth=4.5cm]{14799f21.eps}\includegraphics[width=4.5cm]{14799f22.eps}
\end{figure} Figure 5:

Cross-correlation functions (cross symbols) of the Cepheus moving groups TTS candidates BD+78 853 (RasTyc 0000+7940), TYC 4496-780-1 (RasTyc 0013+7702), TYC 4500-1478-1 (RasTyc 0038+7903), and BD+78 19 (RasTyc 0039+7905) (from left to right) computed from their H$\alpha $ (upper panels) and lithium (lower panels) spectra. The continuous red line displayed in each panel shows the best fit, either with a Gaussian or a rotational profile. The residuals are displayed with a thin black line in the bottom of each panel.

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