Multiple stellar populations in Magellanic Cloud clusters - I. An ordinary feature for intermediate age globulars in the LMC?

A. P. Milone; L. R. Bedin; G. Piotto; J. Anderson

doi:10.1051/0004-6361/200810870

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Volume 497 / No 3 (April III 2009)

A&A, 497 3 (2009) 755-771

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Issue		A&A Volume 497, Number 3, April III 2009


Page(s)		755 - 771
Section		Galactic structure, stellar clusters, and populations
DOI		https://doi.org/10.1051/0004-6361/200810870
Published online		18 February 2009

Online Material

Table 1: Description of the data sets.

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f13.ps} \end{figure}$	Figure 13: As in Fig. 7 for NGC 1987.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f14.ps} \end{figure}$	Figure 14: As in Fig. 7 for NGC 2108.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f15.ps} \end{figure}$	Figure 15: As in Fig. 7 for HODGE 7.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f16.ps} \end{figure}$	Figure 16: As in Fig. 7 for NGC 1852.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f17.ps} \end{figure}$	Figure 17: As in Fig. 7 for NGC 1917.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f18.ps} \end{figure}$	Figure 18: As in Fig. 7 for NGC 2154.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f19.ps} \end{figure}$	Figure 19: As in Fig. 7 for IC 2146.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f20.ps} \end{figure}$	Figure 20: As in Fig. 7 for NGC 1644.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f21.ps} \end{figure}$	Figure 21: As in Fig. 7 for NGC 1652.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f22.ps} \end{figure}$	Figure 22: As in Fig. 7 for NGC 1795.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.75cm]{0870f23.ps} \end{figure}$	Figure 23: As in Fig. 7 for NGC 1978.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=18cm]{0870f32.ps} \end{figure}$	Figure 32: As in Fig. 31 for NGC 1846, NGC 1806, and NGC 1751.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=17cm,clip]{0870f33.ps} \end{figure}$	Figure 33: As in Fig. 31 for NGC 1987, NGC 2108 and ESO057-SC075.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{0870f34.ps} \end{figure}$	Figure 34: As in Fig. 31 for NGC 1783 and NGC 1852.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=17cm,clip]{0870f35.ps} \end{figure}$	Figure 35: As in Fig. 31 for NGC 1975, NGC 1644, and NGC 1652.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=18cm]{0870f36.ps} \end{figure}$	Figure 36: As in Fig. 31 for NGC 1978 and IC 2146.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=17cm,clip]{0870f38.ps} \end{figure}$	Figure 38: As in Fig. 37 for NGC 1652, NGC 1644, NGC 1917, HODGE7, NGC 1852, and NGC 2154.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=17cm,clip]{0870f39.ps} \end{figure}$	Figure 39: As in Fig. 37 for IC 2146, NGC 2108, NGC 1978, and NGC 1795.
Open with DEXTER

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