Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-05-31
Astronomy and Astrophysics
Astrophysics
10 pages, Accepted for publication in the August, 2001 Astronomical Journal
Scientific paper
10.1086/321164
We report new photometry for the cluster NGC 2121 in the Large Magellanic Cloud, which shows a prominent hydrogen core exhaustion gap at the turnoff, and a descending subgiant branch remniscent of Galactic open clusters. We achieve an excellent fit using the Girardi isochrones, finding an age of 3.2 +/- 0.5Gyr, with [Fe/H]=-0.6 +/- 0.2. The isochrones fit the color and shape of the turnoff and subgiant branch so precisely that we constrain the metallicity as well as the age. The smae isochrones also fit SL 663 and NGC 2155, although our photometry for these clusters has much larger errors. We find these clusters to be 0.8 Gyr younger, and 0.4 dex more metal rich, than recently reported in the literature. Consequently, we argue that NGC 2121, NGC 2155, and SL 663 are not properly assigned to the age gap in the LMC, but instead are among the first clusters to have formed int he relatively metal rich, younger group of LMC clusters. We propose a new definition of the LMC Age Gap as extending from 3.2 to 13 Gyr, with ESO121-SCO3 still the only remaining candidate for membership in the age gap.
Rich Robert Michael
Shara Michael M.
Zurek David
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