The question of the abundance of metals in stars with planets

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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.

Keywords: Evolution of stars; Late-type stars; Metal abundances; Stars

Document Type: Research Article


Affiliations: Fesenkov Astrophysical Institute, Almaty, 050020, Kazakhstan

Publication date: August 1, 2005

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