no code implementations • 4 Jan 2021 • S. E. Motta, J. J. E. Kajava, M. Giustini, D. R. A. Williams, M. Del Santo, R. Fender, D. A. Green, I. Heywood, L. Rhodes, A. Segreto, G. Sivakoff, P. A. Woudt
We find that while the X-ray emission remained unprecedentedly low for most of the time following the decline in 2018, the radio emission shows a clear mode change half way through the extended X-ray plateau in 2019 June: from low flux (~3mJy) and limited variability, to marked flaring with fluxes two orders of magnitude larger.
High Energy Astrophysical Phenomena
