The 2018 outburst of BHXB H1743-322 as seen with MeerKAT

In recent years, the black hole candidate X-ray binary system H1743-322 has undergone outbursts and it has been observed with X-ray and radio telescopes. We present 1.3 GHz MeerKAT radio data from the ThunderKAT Large Survey Project on radio transients for the 2018 outburst of H1743-322. We obtain s...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2020-01, Vol.491 (1), p.L29-L33
Hauptverfasser: Williams, D. R. A., Motta, S. E., Fender, R., Bright, J., Heywood, Tremou, E., Woudt, P., Buckley, D. A. H., Corbel, S., Coriat, M., Joseph, T., Rhodes, L., Sivakoff, G. R., van der Horst, A. J.
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Sprache:eng
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Zusammenfassung:In recent years, the black hole candidate X-ray binary system H1743-322 has undergone outbursts and it has been observed with X-ray and radio telescopes. We present 1.3 GHz MeerKAT radio data from the ThunderKAT Large Survey Project on radio transients for the 2018 outburst of H1743-322. We obtain seven detections from a weekly monitoring programme and use publicly available Swift X-ray Telescope and Monitor of All-sky X-ray Image data to investigate the radio/X-ray correlation of H1743-322 for this outburst. We compare the 2018 outburst with those reported in the literature for this system and find that the X-ray outburst reported is similar to previously reported 'hard-only' outbursts. As in previous outbursts, H1743-322 follows the 'radio-quiet' correlation in the radio/X-ray plane for black hole X-ray binaries, and the radio spectral index throughout the outburst is consistent with the 'radio-quiet' population.
ISSN:0035-8711
1745-3925
1365-2966
1745-3933
DOI:10.1093/mnrasl/slz152