Evolution of the recent high-accretion state of the recurrent nova T CrB: HST, Swift, NuSTAR, and XMM-Newton observations

Fuente: arXiv

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Bibliographic Details
Main Authors:	Luna, G. J. M., Kuin, N. P. M., Mukai, K., Sokoloski, J. L., Page, K., Osborne, J. P.
Format:	Preprint
Published:	2026
Subjects:	High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2601.16190