Archibald, R. F.R. F.ArchibaldBURGAY, MARTAMARTABURGAYLyutikov, M.M.LyutikovKaspi, V. M.V. M.KaspiEsposito, P.P.EspositoISRAEL, Gian LucaGian LucaISRAELKerr, M.M.KerrPOSSENTI, ANDREAANDREAPOSSENTIRea, N.N.ReaSarkissian, J.J.SarkissianScholz, P.P.ScholzTendulkar, S. P.S. P.Tendulkar2020-07-272020-07-2720170004-637Xhttp://hdl.handle.net/20.500.12386/26644Rotation-powered pulsars and magnetars are two different observational manifestations of neutron stars: rotation-powered pulsars are rapidly spinning objects that are mostly observed as pulsating radio sources, while magnetars, neutron stars with the highest known magnetic fields, often emit short-duration X-ray bursts. Here, we report simultaneous observations of the high-magnetic-field radio pulsar PSR J1119-6127 at X-ray, with XMM-Newton and NuSTAR, and at radio energies with the Parkes radio telescope, during a period of magnetar-like bursts. The rotationally powered radio emission shuts off coincident with the occurrence of multiple X-ray bursts and recovers on a timescale of ∼70 s. These observations of related radio and X-ray phenomena further solidify the connection between radio pulsars and magnetars and suggest that the pair plasma produced in bursts can disrupt the acceleration mechanism of radio-emitting particles.STAMPAenArticle10.3847/2041-8213/aa93712-s2.0-85034234867000414266100002https://iopscience.iop.org/article/10.3847/2041-8213/aa93712017ApJ...849L..20AFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation