The magnetar Swift J1818.0–1607, discovered in 2020, is one of just 30 other such objects detected in the Milky Way (so far). Swift is rare even among this select few.
Magnetars are supergiant stars that fail to go supernova and instead collapse into ultra-dense cores thanks to their own immense gravity. As opposed to other types of neutron stars which form in similar fashion, magnetars produce extremely powerful magnetic fields, hence the name.
Following a raft of new observations courtesy of the scientists at the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav), researchers found that Swift also emits radio waves, behaving more like a pulsar, another offshoot of neutron stars, which blast out powerful beams of radiation from their poles, rather than a garden-variety magnetar.
Over the course of eight observations in a period of five months throughout 2020, astronomers noticed the radio pulses changed dramatically.
Swift behaved like a pulsar in May, showcased a kind of weak flickering in June, and then displayed a blend of pulsar-like and magnetar-like pulses in July before eventually settling down in August to a more magnetar-like state.