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Monageng, I M; Motta, S E; Fender, R; Yu, W; A Woudt, P; Tremou, E; Miller-Jones, J C A; van der Horst, A J
Monthly notices of the Royal Astronomical Society, 03/2021, Letnik: 501, Številka: 4Journal Article
ABSTRACT We present the results of a weekly monitoring of the new black hole candidate X-ray binary MAXI J1631-472 carried out with the MeerKAT radio interferometer, the Neil Gehrels Swift Observatory, and the Monitor of All-sky X-ray Image (MAXI) instrument, during its 2018–2019 outburst. The source exhibits a number of X-ray states, in particular both high- and low-luminosity hard states bracketed by extended soft states. Radio flaring is observed shortly after a transition from hard/intermediate states to the soft state. This is broadly in agreement with existing empirical models, but its extended duration hints at multiple unresolved flares and/or jet–ISM interactions. In the hard state radio:X-ray plane, the source is revealed to be ‘radio quiet’ at high luminosities, but to rejoin the ‘standard’ track at lower luminosities, an increasingly common observed pattern of behaviour.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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