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Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It Will Be the Brightest Classical or Recurrent Nova Ever Observed in X-Rays

T Coronae Borealis (TCrB) is a recurrent nova with recorded outbursts in 1866 and 1946 and possible outbursts in 1217 and 1787. It is predicted to explode again in 2025 or 2026 based on multiple observational studies. The system consists of a massive ( M _wd  ≳ 1.35 M _⊙ ) white dwarf (WD) and a red...

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Main Authors: S. Starrfield, M. Bose, C. E. Woodward, C. Iliadis, W. R. Hix, A. Evans, G. Shaw, D. P. K. Banerjee, T. Liimets, K. L. Page, T. R. Geballe, I. Ilyin, I. Perron, R. M. Wagner
Format: Artigo
Language:Inglês
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Cataclysmic variable stars
Recurrent novae
Novae
Symbiotic novae
Galaxy chemical evolution
Galaxy abundances
Online Access:https://doi.org/10.3847/1538-4357/adb8ed
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