2001/05/08 by Stuart A. Sim, Stuart Sim · 2 citations
Physics and Astronomy · #Astro and Planetary Science #Solar and Space Plasma Dynamics #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2001.04632.x
published as Mon.Not.Roy.Astron.Soc. 326 (2001) 821 · 14 pages, 10 figures, to be published in MNRAS
arxiv created 2001/05/08 · openalex publication_date 2001/09/01 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/07/28
The modelling of the Lyman lines of hydrogen is extremely important for the study of stellar atmospheres. The Lyman α line is the strongest single line in the ultraviolet spectra of cool stars and represents a significant energy loss