The X-ray counterpart to the gravitational-wave event GW170817

Autor: Eleonora Troja, R. Sanchez-Ramirez, Oleg Korobkin, P. D'Avanzo, Alexander Kutyrev, H. G. Khandrika, Stefano Covino, Y.Y. Yoon, R. E. Ryan, Hyung Mok Lee, G. Lim, H. van Eerten, Myungshin Im, Ryan Wollaeger, Nathaniel R. Butler, Sylvain Veilleux, Roberto Ricci, Luigi Piro, Changsu Choi, A. Y. Lien, Christopher J. Fontes, M. H. Wieringa, Selyeong Lee, Seung-Lee Kim, C.-U. Lee, William H. Lee, Alan M. Watson, O. D. Fox, J. H. Kim, Chris L. Fryer, S. B. Cenko, J. Becerra González, J. M. Burgess, T. Sakamoto

Publikováno v: Troja, E, Piro, L, Eerten, H V, Wollaeger, R T, Im, M, Fox, O D, Butler, N R, Cenko, S B, Sakamoto, T, Fryer, C L, Ricci, R, Lien, A, Jr, R E R, Korobkin, O, Lee, S-K, Burgess, J M, Lee, W H, Watson, A M, Choi, C, Covino, S, Avanzo, P D, Fontes, C J, Gonzalez, J B, Khandrika, H G, Kim, J, Kim, S-L, Lee, C-U, Lee, H M, Kutyrev, A, Lim, G, Sanchez-Ramirez, R, Veilleux, S, Wieringa, M H & Yoon, Y 2017, ' The X-ray counterpart to the gravitational wave event GW 170817 ', Nature, vol. 551, pp. 71-74 . https://doi.org/10.1038/nature24290
Nature

A long-standing paradigm in astrophysics is that collisions- or mergers- of two neutron stars (NSs) form highly relativistic and collimated outflows (jets) powering gamma-ray bursts (GRBs) of short (< 2 s) duration. However, the observational support

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20954a8e87e361a9bff053dcf224dad3
http://hdl.handle.net/20.500.12386/27082