An emission state switching radio transient with a 54 minute period

TL;DR

This paper reports the discovery of a unique long-period radio transient with three emission states, challenging existing models of neutron star emission and suggesting complex physical changes in its source region.

Contribution

It presents the first observation of a long-period radio transient with multiple emission states and mode switching, providing new insights into neutron star-like objects.

Findings

Discovered ASKAP J193505.1+214841 with a 53.8-minute period.

Identified three distinct emission states with different polarizations.

Observed evolution of emission states over 8 months, indicating physical changes.

Abstract

Long-period radio transients are an emerging class of extreme astrophysical events of which only three are known. These objects emit highly polarised, coherent pulses of typically a few tens of seconds duration and minutes to hour-long periods. While magnetic white dwarfs and magnetars, either isolated or in binary systems, have been invoked to explain these objects, a consensus has not emerged. Here we report on the discovery of ASKAP J193505.1+214841.0 (henceforth ASKAPJ1935+2148) with a period of 53.8 minutes exhibiting three distinct emission states - a bright pulse state with highly linearly polarised pulses with widths of 10-50 seconds; a weak pulse state which is about 26 times fainter than the bright state with highly circularly polarised pulses of widths of approximately 370 milliseconds; and a quiescent or quenched state with no pulses. The first two states have been observed to progressively evolve over the course of 8 months with the quenched state interspersed between them suggesting physical changes in the region producing the emission. A constraint on the radius of the source for the observed period rules out a magnetic white dwarf origin. Unlike other long-period sources, ASKAPJ1935+2148 is the first to exhibit drastic variations in emission modes reminiscent of neutron stars. However, its radio properties challenge our current understanding of neutron star emission and evolution.