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X-ray spectroscopy mass constraints on V1674 Her: the fastest nova does not have a near-Chandrasekhar white dwarf

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Olbemo, Tekeba, Errando, Manel, Gokus, Andrea
Format:	Preprint
Publié:	2026
Sujets:	High Energy Astrophysical Phenomena 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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