CCD SDSS Photometry of Poorly Studied Star Clusters in the Large Magellanic Cloud
Figure 7
The ZAMS and three isochrones ( = 0.008) from Marigo et al. [10] superimposed to LMC cluster CMDs. The youngest isochrone corresponds to log() − (log()) (see Table 3), whereas the isochrone separation is (log()) = 0.10.
