SPAMMS: 3D spectroscopic modeling of stellar surfaces. II. Implementation of Kurucz and TLUSTY model atmospheres

arXiv:2609.15331 · astro-ph.SR, astro-ph.EP · Submitted 2026-09-14 · Read on arXiv

astro-ph.SR, astro-ph.EP

Submitted: 2026-09-14

Updated: 2026-09-23

Comments: Accepted for publication in A&A; 12 pages (+3 appendix pages), 7 figures (+3 appendix figures)

Code: https://github.com/DGalanDieguez/PRISMAS

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

Terminology

• Abundance — 11× in this paper · explained in 1 episode
• Metallicity — 7× in this paper · explained in 3 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Core — 1× in this paper · explained in 2 episodes

Sources

• TLUSTY and SYNSPEC Users's Guide IV: Upgraded Versions 208 and 54
• A brief introductory guide to TLUSTY and SYNSPEC
• TLUSTY User's Guide II: Reference Manual
• TLUSTY User's Guide III: Operational Manual
• Multiplicity of Massive stars in the Milky Way (M3W). I. Project description, UNWIND, application to GLS 11 448, and DIB catalog
• Stellar Atmospheres
• Observational constraints on massive binaries

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Constraining the origin of magnetic white dwarfs
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
• Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
• Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?