Hydrogen Atom Collision Processes in Cool Stellar Atmospheres: Effects on Spectral Line Strengths and Measured Chemical Abundances in Old Stars
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
http://stacks.iop.org/1742-6596/397/i=1/a=012049/pdf
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1. Mutual Neutralization in Li++H−/D− and Na++H−/D− Collisions: Implications of Experimental Results for Non-LTE Modeling of Stellar Spectra;The Astrophysical Journal;2021-02-01
2. Spectroscopic and structural investigation for the ground and excited states of CaNa+ molecular ion;Journal of Quantitative Spectroscopy and Radiative Transfer;2018-04
3. Low-energy inelastic atomic collisions of magnesium and hydrogen;Russian Journal of Physical Chemistry B;2017-01
4. Model estimates of inelastic calcium-hydrogen collision data for non-LTE stellar atmospheres modeling;Astronomy & Astrophysics;2016-02-26
5. Inelastic cross sections for low-energy Mg + H collisions;Journal of Physics: Conference Series;2014-12-10
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