Discovery of Powerful Gamma-Ray Flares from the Crab Nebula

Autor: F. Fuschino, Craig O. Heinke, M. Pilia, A. Argan, G. Di Cocco, P. Giommi, Francesco Longo, Fulvio Gianotti, Andrea Bulgarelli, C. Pittori, A. Zambra, Enrico Costa, Guido Barbiellini, Dieter Horns, Carlo Ferrigno, V. Vittorini, M. Trifoglio, Riccardo Campana, M. Prest, Ennio Morelli, E. Striani, F. Perotti, G. Piano, Y. Evangelista, Paolo Lipari, P. Santolamazza, T. Contessi, M. Giusti, Francesco Lazzarotto, Giovanni F. Bignami, Alda Rubini, P. W. Cattaneo, Arnaud Ferrari, D. Zanello, I. Lapshov, Marco Tavani, S. Sabatini, Claudio Labanti, Alessio Trois, Marco Feroci, Luigi Pacciani, Martino Marisaldi, A. De Luca, A. W. Chen, F. Lucarelli, E. Del Monte, L. Salotti, P. A. Caraveo, A. Pellizzoni, A. Morselli, G. DeParis, Martin C. Weisskopf, Allyn F. Tennant, Elena Moretti, M. Galli, P. Picozza, A. Giuliani, A. Rappoldi, E. Vallazza, Sandro Mereghetti, G. Pucella, Massimo Rapisarda, F. Verrecchia, I. Donnarumma, G. Di Persio, Filippo D'Ammando, Paolo Soffitta, S. Vercellone

Publikováno v: Science. 331:736-739

The well known Crab Nebula is at the center of the SN1054 supernova remnant. It consists of a rotationally-powered pulsar interacting with a surrounding nebula through a relativistic particle wind. The emissions originating from the pulsar and nebula

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6607b61e7143246c88c1c270eb46395
https://doi.org/10.1126/science.1200083