Strange neutron star spinning every 76 seconds discovered in stellar graveyard
The newly discovered neutron star is named, PSR J0901-4046, and shows characteristics of pulsars, (ultra-long period) magnetars and even fast radio bursts. While the radio energy produced suggests a pulsar origin, the pulses with chaotic sub-pulse components, and the polarization of the pulses are reminiscent of magnetars.
While the spin period of PSR J0901−4046 might be more consistent with a white dwarf, another less extreme type of stellar remnant, scientists do not see any multi-wavelength support for this. It is presently unclear how long this source has been emitting in the radio. It was discovered in a well-studied part of the galaxy, but radio surveys don’t usually search for periods this long, or pulses that last more than a few tens of milliseconds.
“The radio emission from this neutron star is unlike any we have ever seen before,” explained Professor Ben Stappers at The University of Manchester and Principal Investigator of the MeerTRAP project. “We get to view it for about 300 milliseconds, which is much longer than for the majority of other radio emitting neutron stars. There seem to be at least 7 different pulse types, some of which show strongly periodic structure, which could be interpreted as seismic vibrations of the neutron star. These pulses might be giving us vital insight into the nature of the emission mechanism for these sources.”
“The sensitivity that MeerKAT provides, combined with the sophisticated searching that was possible with MeerTRAP and an ability to make simultaneous images of the sky made this discovery possible. Even then it took an eagle eye to recognise it for something that was possibly a real source because it was so unusual looking!” said Dr Ian Heywood from the ThunderKAT team and the University of Oxford who collaborated on this study.
Detecting similar sources is observationally challenging, which implies that there may be a larger undetected population waiting to be uncovered. This new discovery adds to the possibility of the existence of a new class of radio transients, the ultra-long period neutron stars, suggesting a possible connection to the evolution of highly magnetized neutron stars, ultra-long period magnetars, and fast radio bursts.
The paper, ‘Discovery of a radio-emitting neutron star with an ultra-long spin period of 76s’, is published in Nature Astronomy .