A New Approach to Modeling Line Shapes with Quasi-H 2+ Satellites in Stellar Atmospheres

arXiv:2607.28920 · astro-ph.SR, physics.atom-ph · Submitted 2026-07-31 · Read on arXiv

Jackson R. White, Thomas A. Gomez, Mark C. Zammit, Michael H. Montgomery, Bart H. Dunlap, Ivan Hubeny, Dmitry V. Fursa, Igor Bray, Don E. Winget

astro-ph.SR, physics.atom-ph

Submitted: 2026-07-31

Comments: 20 pages, 15 figures, accepted by ApJ

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 22× in this paper · explained in 2 episodes
• Unified Line Broadening Theory — 3× in this paper
• Abundance — 2× in this paper · explained in 1 episode
• Trace — 2× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Hilbert Space — 1× in this paper · explained in 2 episodes

Sources

• TLUSTY and SYNSPEC Users's Guide IV: Upgraded Versions 208 and 54

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