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Autor:
Michael Kolacki, Luke F. Roberts, Tanmayee Gupte, Scott C. Noble, Leonardo R. Werneck, Ariadna Murguia-Berthier, Manuela Campanelli, Julian H. Krolik, Jeremy D. Schnittman, Jesus M. Rueda-Becerril, Lorenzo Ennoggi, Grace Fiacco, Bernard J. Kelly, Brendan Drachler, Joshua A. Faber, Riccardo Ciolfi, Bruno Giacomazzo, Yosef Zlochower, Richard O'Shaughnessy, Yossef Zenati, Enrico Ramirez-Ruiz, Ben Margalit, Federico Cipolletta, Mark J. Avara, Zachariah B. Etienne, Federico G. Lopez Armengol, Trung Ha, Tim Moon
The first binary neutron star merger has already been detected in gravitational waves. The signal was accompanied by an electromagnetic counterpart including a kilonova component powered by the decay of radioactive nuclei, as well as a short $\gamma$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2872099cc845c2bbd7a2401ab9ac60e
http://hdl.handle.net/10281/336199
http://hdl.handle.net/10281/336199