Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26at...24..335k&link_type=abstract
Astronomical and Astrophysical Transactions, vol. 24, Issue 4, p.335-341
Astronomy and Astrophysics
Astronomy
Stars, Metal Abundances, Late-Type Stars, Evolution Of Stars
Scientific paper
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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