A statistical framework for the quantitative spectroscopy of luminous blue stars

Context. Quantitative spectroscopy of luminous blue stars relies on detailed non-local thermodynamic equilibrium (non-LTE) model atmospheres whose increasing physical realism makes direct iterative analyses computationally demanding. Aims. We introduce Machine-learning assisted Uncertainty inference...

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Detalles Bibliográficos

Autor Principal:	Urbaneja M. A.
Formato:	Artigo
Idioma:	Inglês
Publicado:	EDP Sciences 2026-03-01
Series:	Astronomy & Astrophysics
Assuntos:	methods: statistical techniques: spectroscopic stars: atmospheres stars: early-type stars: fundamental parameters
Acceso en liña:	https://www.aanda.org/articles/aa/full_html/2026/03/aa58001-25/aa58001-25.html
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