The Influence of Chemi-Ionization and Recombination Processes on Spectral Line Shapes in Stellar Atmospheres
The chemi-ionization processes in atom - Rydberg atom collisions, as well as the corresponding chemi-recombination processes, are considered as factors of influence on the atom exited-state populations in weakly ionized layers of stellar atmospheres.The presented results are related to the photospheres of the Sun and some M red dwarfs, as well as w