Discovery of “isolated” co-moving T Tauri stars in Cepheus

P. Guillout; A. Frasca; A. Klutsch; E. Marilli; D. Montes

doi:10.1051/0004-6361/201014799

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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