# Rapidly evolving disk-jet coupling during re-brightenings in the black hole transient MAXI J1535-571

## TL;DR

This study investigates the rapid evolution of disk-jet coupling during multiple re-brightenings in the black hole binary MAXI J1535-571, revealing faster changes in accretion and jet behavior than typically observed.

## Contribution

It provides the first detailed analysis of disk-jet coupling during multiple rapid re-brightenings in a black hole low-mass X-ray binary, highlighting faster evolution timescales.

## Key findings

- Re-brightenings show high peak X-ray luminosity and state transitions.
- Compact radio jets are brightened and quenched in tandem with X-ray state changes.
- Accretion flow and jet properties evolve on days, not weeks, during re-brightenings.

## Abstract

The main outburst of the candidate black hole low-mass X-ray binary (BH LMXB) MAXI J1535-571 ended in 2018 May and was followed by at least five episodes of re-brightenings. We have monitored this re-brightening phenomenon at X-ray and radio wavelengths using the {\it Neil Gehrels Swift Observatory} and Australia Telescope Compact Array, respectively. The first two re-brightenings exhibited a high peak X-ray luminosity (implying a high mass accretion rate) and were observed to transition from the hard to the soft state. However, unlike the main outburst, these re-brightenings did not exhibit clear hysteresis. During the re-brightenings, when MAXI J1535-571 was in the hard state, we observed the brightening of a compact radio jet which was subsequently quenched when the source transitioned to a similar soft state as was observed during the main outburst. We report on the first investigation of disk-jet coupling over multiple rapidly evolving re-brightenings in a BH LMXB. We find that the accretion flow properties and the accompanying compact jet evolve on a similarly rapid time scale of ~days rather than the typical value of ~weeks as observed for most other BH LMXBs during their main outburst events.