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Machine learning for understanding pulsating stars I: the non-linear phenomenon in δ Scuti stars

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Rodon, J. R., Pascual-Granado, J., Lares-Martiz, M., Sánchez, M. Rodríguez, Roche, C.
Format:	Preprint
Publié:	2026
Sujets:	Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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