The question of the abundance of metals in stars with planets
The metal-poor stars with planets were compared with the metal-rich stars also with planets. The high [Fe]/[H] values obtained from the spectroscopic analysis for most stars with planets can be consequence of the fact that the models used are inadequate for real stellar atmospheres.
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Document Type: Research Article
Affiliations: Fesenkov Astrophysical Institute, Almaty, 050020, Kazakhstan
Publication date: 2005-08-01