Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It will be the Brightest Classical or Recurrent Nova Ever Observed in X-rays

Fuente: arXiv

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Bibliographic Details
Main Authors:	Starrfield, S., Bose, M., Woodward, C. E., Iliadis, C., Hix, W. R., Evans, A., Shaw, G., Banerjee, D. P. K., Liimets, T., Page, K. L., Geballe, T. R., Ilyin, I., Perron, I., Wagner, R. M.
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2502.10925