The Influence of Chemi-Ionization and Recombination Processes on Spectral Line Shapes in Stellar Atmospheres

Articles in the same Issue

1. Stark Broadening and White Dwarfs
2. VAMDC as a Resource for Atomic and Molecular Data and the New Release of VALD
3. Stark Broadening of Carbon and Oxygen Lines in Hot DQ White Dwarf Stars: Recent Results and Applications
4. Recent Results for Widths of Lines Important in the Spectra of Cool Stars
5. Comparisons and Comments on Electron and Ion Impact Profiles of Spectral Lines
6. Optical Spectroscopy with the Technology of Virtual Observatory
7. Stochastic Processes Applied to Line Shapes
8. A Statistical Study of the Si IV Resonance Line Parameters in 19 Be Stars
9. Ab Initio Determination of Atomic Structure and Stark Broadening Parameters: Pb IV and Recent Results
10. Analysis of Hydrogen Cyanide Hyperfine Spectral Components towards Star Forming Cores
11. The Influence of Chemi-Ionization and Recombination Processes on Spectral Line Shapes in Stellar Atmospheres
12. Studying the UV Mg II Resonance Lines in 20 Be Stars
13. Stark Broadening of Several Ar I Spectral Lines in the Visible Spectrum
14. Stark Broadening of Several Ne II, Ne III and O III Spectral Lines for the Stark-B Database
15. Cross Sections for Electron Impact Excitation of O VI Lines
16. Diagnostics of the Solar X-Flare Impact on Lower Ionosphere through the VLF-NAA Signal Recordings
17. Statistical Analysis of Langmuir Waves Associated with Type III Radio Bursts: I. Wind Observations
18. Statistical Analysis of Langmuir Waves Associated with Type III Radio Bursts: II. Simulation and Interpretation of the Wave Energy Distributions
19. Modeling of the Continuous Absorption of Electromagnetic Radiation in Dense Hydrogen Plasma
20. The Influence of Solar Spectral Lines on Electron Concentration in Terrestrial Ionosphere
21. Stark Broadening of In III Lines in Astrophysical and Laboratory Plasma
22. Plasmas Generated with Gas Mixtures at the Atmospheric Pressure
23. On the Gas Temperature Determination from Van Der Waals Broadening in Argon - Neon Microwave Plasmas