PSR J0026-1955: A curious case of evolutionary subpulse drifting and nulling

TL;DR

This paper analyzes PSR J0026-1955, a pulsar exhibiting complex subpulse drifting, nulling, and mode changes, providing new observational insights and proposing models for its drift rate evolution, thus advancing understanding of pulsar emission physics.

Contribution

It presents detailed observations of PSR J0026-1955's drifting modes, nulling behavior, and drift rate evolution, and introduces models explaining the observed drift rate changes.

Findings

Identified two distinct drifting modes, A and B, with subcategories.

Estimated nulling fraction of ~58%, lower than previous reports.

Evidence of subpulse memory across nulls and mode A2 often followed by null.

Abstract

PSR J0026-1955 was independently discovered by the Murchison Widefield Array (MWA) recently. The pulsar exhibits subpulse drifting, where the radio emission from a pulsar appears to drift in spin phase within the main pulse profile, and nulling, where the emission ceases briefly. The pulsar showcases a curious case of drift rate evolution as it exhibits rapid changes between the drift modes and a gradual evolution in the drift rate within a mode. Here we report new analysis and results from observations of J0026-1955 made with the upgraded Giant Meterwave Radio Telescope (uGMRT) at 300-500 MHz. We identify two distinct subpulse drifting modes: A and B, with mode A sub-categorised into A0, A1, and A2, depending upon the drift rate evolutionary behaviour. Additionally, the pulsar exhibits short and long nulls, with an estimated overall nulling fraction of ~58%, which is lower than the previously reported value. Our results also provide evidence of subpulse memory across nulls and a consistent behaviour where mode A2 is often followed by a null. We investigate the drift rate modulations of J0026-1955 and put forward two different models to explain the observed drifting behaviour. We suggest that either a change in polar gap screening or a slow relaxation in the spark configuration could possibly drive the evolution in drift rates. J0026-1955 belongs to a rare subset of pulsars which exhibit subpulse drifting, nulling, mode changing, and drift rate evolution. It is, therefore, an ideal test bed for carousel models and to uncover the intricacies of pulsar emission physics.