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EP250207b is not a collapsar fast X-ray transient. Is it due to a compact object merger?

Fuente: arXiv

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Bibliographic Details
Main Authors:	Jonker, P. G., Levan, A. J., Liu, Xing, Xu, Dong, Liu, Yuan, Xu, Xinpeng, Li, An, Sarin, N., Tanvir, N. R., Lamb, G. P., Ravasio, M. E., Sánchez-Sierras, J., Quirola-Vásquez, J. A., Rayson, B. C., van Dalen, J. N. D., Malesani, D. B., van Hoof, A. P. C., Bauer, F. E., Chacón, J., Smartt, S. J., Martin-Carrillo, A., Corcoran, G., Cotter, L., Rossi, A., Onori, F., Fraser, M., O'Brien, P. T., Eyles-Ferris, R. A. J., Hjorth, J., Chen, T. -W., Leloudas, G., Tomasella, L., Schulze, S., De Pasquale, M., Carotenuto, F., Bright, J., Wang, Chenwei, Xiong, Shaolin, Zhang, Jinpeng, Xue, Wangchen, Liu, Jiacong, Li, Chengkui, Sanchez, D. Mata, Torres, M. A. P.
Format:	Preprint
Published:	2025
Subjects:	High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2508.13039