no code implementations • 3 Dec 2020 • Ersin Gogus, Matthew G. Baring, Chryssa Kouveliotou, Tolga Guver, Lin Lin, Oliver J. Roberts, George Younes, Yuki Kaneko, Alexander J. van der Horst
Our investigations of the XMM-Newton and Chandra spectra with a variety of phenomenological and physically-motivated models, concluded that the magnetic field topology of SGR J1935+2154 is most likely highly non-dipolar.
High Energy Astrophysical Phenomena
