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arXiv · 1906.01000

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

A. S. Parikh·T. D. Russell·R. Wijnands·J. C. A. Miller-Jones·G. R. Sivakoff·A. J. Tetarenko
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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.

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A. S. Parikh, T. D. Russell, R. Wijnands, J. C. A. Miller-Jones, G. R. Sivakoff, A. J. Tetarenko. 2019-06-03. Rapidly evolving disk-jet coupling during re-brightenings in the black hole transient MAXI J1535-571. https://doi.org/10.3847/2041-8213/ab2636

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