The binary neutron star merger event GW170817 was detected through both electromagnetic radiation and gravitational waves. Its afterglow emission may have been produced by either a narrow relativistic jet or an isotropic outflow. High-spatial-resolution measurements of the source size and displaceme...
Bibliographic Details
| Authors: |
Ghirlanda, G.;
Salafia, O.S.;
Paragi, Z.;
Giroletti, M.;
Yang, J.;
Marcote, B.;
Blanchard, J.;
Agudo, I.;
An, T.;
Bernardini, M.G.;
Beswick, R.;
Branchesi, M.;
Campana, S.;
Casadio, C.;
Chassande-Mottin, E.;
Colpi, M.;
Covino, S.;
D''Avanzo, P.;
D''Elia, V.;
Frey, S.;
Gawronski, M.;
Ghisellini, G.;
Gurvits, L.I.;
Jonker, P.G.;
Van Langevelde, H.J.;
Melandri, A.;
Moldon, J.;
Nava, L.;
Perego, A.;
Perez-Torres, M.A.;
Reynolds, C.;
Salvaterra, R.;
Tagliaferri, G.;
Venturi, T.;
Vergani, S.D.;
Zhang, M. |
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| Format: | Article
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| Status: | Accepted version |
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| Publication date: | 2019 |
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| Country: | España |
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| Institution: | Universidad de Zaragoza |
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| Repository: | Zaguán. Repositorio Digital de la Universidad de Zaragoza |
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| OAI Identifier: | oai:zaguan.unizar.es:78946 |
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| Online Access: | http://zaguan.unizar.es/record/78946
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| Access Level: | Open access |
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