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Autor:
Fernández, J. F. Agüí, Thöne, C. C., Kann, D. A., Postigo, A. de Ugarte, Selsing, J., Schady, P., Yates, R. M., Greiner, J., Oates, S. R., Malesani, D., Xu, D., Klotz, A., Campana, S., Rossi, A., Perley, D. A., Blazek, M., D'Avanzo, P., Giunta, A., Hartmann, D., Heintz, K. E., Jakobsson, P., Kirkpatrick IV, C. C., Kouveliotou, C., Melandri, A., Pugliese, G., Salvaterra, R., Starling, R. L. C., Tanvir, N. R., Vergani, S. D., Wiersema, K.
Short Gamma-Ray Bursts (SGRBs) are produced by the coalescence of compact binary systems which are remnants of massive stars. GRB 160410A is classified as a short-duration GRB with extended emission and is currently the farthest SGRB with a redshift
Externí odkaz:
http://arxiv.org/abs/2109.13838