# Disk-jet coupling in the 2017/2018 outburst of the Galactic black hole candidate X-ray binary MAXI J1535-571

## TL;DR

This study provides detailed radio and X-ray observations of MAXI J1535-571 during its 2017/2018 outburst, revealing jet evolution, quenching, and ejection timing related to spectral state transitions.

## Contribution

It offers the first comprehensive radio monitoring of MAXI J1535-571, constraining jet properties and ejection timing in relation to X-ray state changes.

## Key findings

- Detected and tracked a relativistic jet knot for 303 days.
- Constrained the jet inclination to ≤45° and speed to ≥0.69c.
- Identified jet ejection close to spectral state transition.

## Abstract

MAXI J1535-571 is a Galactic black hole candidate X-ray binary that was discovered going into outburst in 2017 September. In this paper, we present comprehensive radio monitoring of this system using the Australia Telescope Compact Array (ATCA), as well as the MeerKAT radio observatory, showing the evolution of the radio jet during its outburst. Our radio observations show the early rise and subsequent quenching of the compact jet as the outburst brightened and then evolved towards the soft state. We constrain the compact jet quenching factor to be more than 3.5 orders of magnitude. We also detected and tracked (for 303 days) a discrete, relativistically-moving jet knot that was launched from the system. From the motion of the apparently superluminal knot, we constrain the jet inclination (at the time of ejection) and speed to $\leq 45^{\circ}$ and $\geq0.69$c, respectively. Extrapolating its motion back in time, our results suggest that the jet knot was ejected close in time to the transition from the hard intermediate state to soft intermediate state. The launching event also occurred contemporaneously with a short increase in X-ray count rate, a rapid drop in the strength of the X-ray variability, and a change in the type-C quasi-periodic oscillation (QPO) frequency that occurs $>$2.5 days before the first appearance of a possible type-B QPO.