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• W2074895149 abstract "The precise measurement of the chemical composition of stars is a fundamental problem relevant to many areas of astrophysics. State-of-the-art approaches attempt to unite accurate descriptions of microphysics, non-local thermodynamic equilibrium (non-LTE) line formation and 3D hydrodynamical model atmospheres. In this paper I review progress in understanding inelastic collisions of hydrogen atoms with other species and their influence on spectral line formation and derived abundances in stellar atmospheres. These collisions are a major source of uncertainty in non-LTE modelling of spectral lines and abundance determinations, especially for old, metal-poor stars, which are unique tracers of the early evolution of our galaxy." @default.
• W2074895149 created "2016-06-24" @default.
• W2074895149 creator A5089867853 @default.
• W2074895149 date "2012-12-06" @default.
• W2074895149 modified "2023-10-17" @default.
• W2074895149 title "Hydrogen Atom Collision Processes in Cool Stellar Atmospheres: Effects on Spectral Line Strengths and Measured Chemical Abundances in Old Stars" @default.
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• W2074895149 doi "https://doi.org/10.1088/1742-6596/397/1/012049" @default.
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