2004/09/14 by Jorge Melendez, J. Meléndez, Melendez, Jorge +3
Earth and Planetary Sciences · Materials Science · Physics and Astronomy · #Astrophysics (astro-ph) #Crystal Structures and Properties #FOS: Physical sciences #High-pressure geophysics and materials #Mineralogy and Gemology Studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0409347
Proceedings, Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, in honor of Dr. David Lambert's 65th birthday, June 17-19, 2004. ASP Conference Series. Edited by F. N. Bash & T. G. Barnes
arxiv created 2004/09/14 · openalex publication_date 2004/09/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We analyze twenty five nearby metal-rich G and late-F dwarfs in order to verify whether the spectroscopic equilibrium (LTE) of iron lines satisfy the observational constraints imposed by the Infrared Flux Method (angular diameters) and Hipparcos parallaxes. The atmospheric parameters derived from iron lines (assuming LTE and employing 1D Kurucz model atmospheres) do not satisfy simultaneously both observational constraints, probably because classical modeling fails to reproduce the detailed line formation of FeI lines.