# Peculiar outbursts of an ultra luminous source likely signs of an aperiodic disc-wind

## TL;DR

This paper reports the discovery of unusual, recurring X-ray bursts from an ultra luminous source in a globular cluster, suggesting an aperiodic disc wind driven by hyper-Eddington accretion as the cause.

## Contribution

It presents the first observation of recurring, aperiodic X-ray bursts from an ultra luminous source, proposing a novel disc wind mechanism driven by hyper-Eddington accretion.

## Key findings

- Discovery of two peculiar X-ray bursts lasting hours.
- Recurrent bursts separated by days, unprecedented in such sources.
- Proposed aperiodic disc wind driven by hyper-Eddington accretion as explanation.

## Abstract

The metal rich globular cluster RZ 2109 in the massive Virgo elliptical galaxy NGC 4472 (M49) harbours the ultra luminous X-ray source XMMU 122939.7+075333. Previous studies showed that this source varies between bright and faint phases on timescales of just a few hours. Here, we report the discovery of two peculiar X-ray bursting events that last for about 8 and 3.5 hours separated by about 3 days. Such a recurring X-ray burst-like behaviour has never been observed before. We argue that type-I X-ray bursts or super bursts as well as outburst scenarios requiring a young stellar object are highly unlikely explanations for the observed light curve, leaving an aperiodic disc wind scenario driven by hyper-Eddington accretion as a viable explanation for this new type of X-ray flaring activities.