Non-LTE line formation for Si I-II-III in A-B stars and the origin of Si II emission lines in iota Her
A comprehensive model atom was developed for Si I-II-III using the most up-to-date atomic data available so far. Based on the non-local thermodynamic equilibrium (non-LTE = NLTE) line formation for Si I, Si II, and Si III and high-resolution observed spectra, we determined the NLTE abundances for a...
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Published in | arXiv.org |
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Main Author | |
Format | Paper Journal Article |
Language | English |
Published |
Ithaca
Cornell University Library, arXiv.org
03.03.2020
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Subjects | |
Online Access | Get full text |
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