The influence of electron collisions on non-LTE Li line formation in stellar atmospheres
The influence of the uncertainties in the rate coefficient data for electron-impact excitation and ionization on non-LTE Li line formation in cool stellar atmospheres is investigated. We examine the electron collision data used in previous non-LTE calculations and compare them to our own calculations using the R-matrix with pseudostates (RMPS) method and to other calculations found in the literature.
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|Source:||Journal of Physics: Conference Series|
|01_Osorio_The_influence_of_electron_2012.pdf||352.95 kB||Adobe PDF||Request a copy|
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