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Analyzing Starbursts Using Magellanic Cloud Star Clusters as Simple Stellar Populations

  • Authors: Andrew J. Leonardi and James A. Rose

Leonardi & Rose 2003 The Astronomical Journal 126 1811.

  • Provider: AAS Journals

Caption: Fig. 16.

Hδ/Fe I λ4045 vs. BD for [Fe/H] = −1.7. The trajectories are the same as in Fig. 10, but now the MC cluster index data are included. Clusters are placed on this and the subsequent BD figures based on their literature metallicity values given in Table 2. The dotted line is the trajectory for [Fe/H] = −0.4 with ages displayed as small labels, while the solid line is the track for [Fe/H] = −1.7 with large labels to mark the ages. All labelled ages are in gigayears. Again, NGC 2210 and NGC 1754 occupy similar regions of the diagram as M15 and M79.

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