Permitted Oxygen Abundances and the Temperature Scale of Metal-poor Turnoff Stars
We use high-quality VLT/UVES published data of the permitted O I triplet and Fe II lines to determine oxygen and iron abundances in unevolved (dwarfs, turnoff, subgiants) metal-poor halo stars. The calculations have been performed both in LTE and non-LTE
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|Source:||Astrophysical Journal, The|
|01_Melendez Moreno_Permitted_Oxygen_Abundances_2006.pdf||482.94 kB||Adobe PDF||Request a copy|
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