Issue |
EAS Publications Series
Volume 43, 2010
Non-LTE Line Formation for Trace Elements in Stellar Atmospheres
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Page(s) | 215 - 222 | |
DOI | https://doi.org/10.1051/eas/1043016 | |
Published online | 16 November 2010 |
Non-LTE Line Formation for Trace Elements in Stellar Atmospheres
R. Monier, B. Smalley, G. Wahlgren and Ph. Stee (eds)
EAS Publications Series, 43 (2010) 215-222
R. Monier, B. Smalley, G. Wahlgren and Ph. Stee (eds)
EAS Publications Series, 43 (2010) 215-222
Departures from lte in chemically stratified atmospheres
Institute of Astronomy, Russian
Academy of Science, Pyatnitskaya
48, 119017
Moscow,
Russia
e-mail: lima@inasan.ru
Two astrophysical problems are reviewed where non-LTE line formation for the selected atoms is considered in a chemically stratified atmosphere and this leads to better interpretation of observed data. These are an origin of the Mn ii emission lines in the 3He and HgMn stars and a violation of the ionization equilibrium between the second and first ions of rare-earth elements in rapidly oscillating chemically peculiar stars.
© EAS, EDP Sciences 2010