# On the connection between radiative outbursts and timing irregularities in magnetars

## TL;DR

This study investigates the relationship between radiative outbursts and timing irregularities in magnetars, revealing that larger glitches are more likely to trigger outbursts, though not all glitches lead to such events.

## Contribution

It provides a systematic analysis of the correlation between glitches and outbursts in magnetars, highlighting the bimodal distribution of glitch sizes and the likelihood of larger glitches inducing outbursts.

## Key findings

- Glitch sizes in magnetars show a bimodal distribution.
- Only 30% of glitches are associated with outbursts.
- Larger glitches tend to induce outbursts more often.

## Abstract

Magnetars are strongly magnetized pulsars and they occasionally show violent radiative outbursts. They also often exhibit glitches which are sudden changes in the spin frequency. It was found that some glitches were associated with outbursts but their connection remains unclear. We present a systematic study to identify possible correlations between them. We find that the glitch size of magnetars likely shows a bimodal distribution, different from the distribution of the Vela-like recurrent glitches but consistent with the high end of that of normal pulsars. A glitch is likely a necessary condition for an outburst but not a sufficient condition because only 30\% of glitches were associated with outbursts. In the outburst cases, the glitches tend to induce larger frequency changes compared to those unassociated ones. We argue that a larger glitch is more likely to trigger the outburst mechanism, either by reconfiguration of the magnetosphere or deformation of the crust. A more frequent and deeper monitoring of magnetars is necessary for further investigation of their connection.