Worldwide astronomical and astrophysical research
| 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 | |
![\begin{figure}
\par\includegraphics[width=4.5cm]{14799f15.eps}\includegraphics[w...
...dth=4.5cm]{14799f21.eps}\includegraphics[width=4.5cm]{14799f22.eps}
\end{figure}](/articles/aa/olm/2010/12/aa14799-10/img80.png)
|
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 |
| Open with DEXTER | |
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(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.