vix.ing · top · new · best · stats · spec

Lithium abundances of halo dwarfs based on excitation temperature

2008/10/30 by A. Hosford, S. G. Ryan, Sean G. Ryan +6 · 1 citation
Physics and Astronomy · #Abundance (ecology) #Anisotropy #Astro and Planetary Science #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Biology #CMB cold spot #Context (archaeology) #Cosmic microwave background #Ecology #Galactic halo #Geology #Halo #Lithium (medication) #Physics #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:200810240

13 pages, 9 figures

openalex publication_date 2008/10/30 · arxiv created 2008/11/15 · arxiv updated 2009/12/01 · openalex created_date 2022/05/12 · openalex updated_date 2026/08/05

Abstract

Context. The discovery of the Spite plateau in the abundances of for metal-poor stars led to the determination of an observationally deduced primordial lithium abundance. However, after the success of the Wilkinson Microwave Anisotropy Probe (WMAP) in determining the baryon density, , there was a discrepancy between observationally determined and theoretically determined abundances in the case of . One of the most important uncertain factors in the calculation of the stellar abundance is the effective temperature, .

Citations

Cited by