2006/09/25 by P. S. Barklem · 6 citations
Engineering · Physics and Astronomy · #Astrophysics and Star Formation Studies #Atomic and Molecular Physics #Atomic electron transition #Atomic oxygen #Excitation #Excited state #Interpretation (philosophy) #Laser-induced spectroscopy and plasma #Oxygen #Stellar atmosphere #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066341
Accepted for A&A; 9 pages, 2 figures, 6 tables
arxiv created 2006/09/25 · openalex publication_date 2006/11/02 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims.Our goal was to calculate transition rates from ground and excited states in neutral oxygen atoms due to electron collisions for non-LTE modelling of oxygen in late-type stellar atmospheres, thus enabling the reliable interpretation of oxygen lines in stellar spectra.