Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-05-09
Astrophys.J. 626 (2005) L49-L52
Astronomy and Astrophysics
Astrophysics
Astrophysical Journal Letters, in press
Scientific paper
10.1086/431668
We present the initial results of a study of the surface lithium abundance in a sample of low-mass members (M~0.4-1.0 Msun) of the Orion Nebula Cluster (ONC) that provide an independent clock to estimate stellar ages. We report discovery of significant depletion of lithium in four stars with estimated mass of ~0.4 Msun and age ~10Myr. Comparison with the predictions of numerical and analytical models shows excellent agreement between the isochronal age and lithium depletion time scale for two objects, the first case in lithium-poor pre-main sequence stars. Our results bear on the issue of the real age spread in the ONC and hence on the overall duration of the star formation process, indicating that the stellar population did not came into existence in a single, rapid burst.
Flaccomio Ettore
Palla Fabrizio
Pallavicini Roberto
Randich Sofia
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