... PHL 1226

Based on observations obtained at the German-Spanish Astronomical Center, Calar Alto, operated by the Max-Planck-Institut für Astronomie Heidelberg jointly with the Spanish National Commission for Astronomy.

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... previously

The larger solar O abundance in Holweger (2001) compared to that derived in Asplund et al. (2004) is due to an ignored contribution from a Ni blend, but also a difference between their adopted 1D and 3D models.

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