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Non-LTE Line Formation in the Near-IR: Hot Stars

Published 2 Dec 2010 in astro-ph.SR | (1012.0605v1)

Abstract: Line-formation calculations in the Rayleigh-Jeans tail of the spectral energy distribution are complicated by an amplification of non-LTE effects. For hot stars this can make quantitative modelling of spectral lines in the near-IR challenging. An introduction to the modelling problems is given and several examples in the context of near-IR line formation for hydrogen and helium are discussed.

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