SIMBAD references

2017ApJ...848...92P - Astrophys. J., 848, 92-92 (2017/October-3)

Up and down the black hole radio/X-Ray correlation: the 2017 mini-outbursts from Swift J1753.5-0127.

PLOTKIN R.M., BRIGHT J., MILLER-JONES J.C.A., SHAW A.W., TOMSICK J.A., RUSSELL T.D., ZHANG G.-B., RUSSELL D.M., FENDER R.P., HOMAN J., ATRI P., BERNARDINI F., GELFAND J.D., LEWIS F., CANTWELL T.M., CAREY S.H., GRAINGE K.J.B., HICKISH J., PERROTT Y.C., RAZAVI-GHODS N., SCAIFE A.M.M., SCOTT P.F. and TITTERINGTON D.J.

Abstract (from CDS):

The candidate black hole X-ray binary Swift J1753.5-0127 faded to quiescence in 2016 November after a prolonged outburst that was discovered in 2005. Nearly three months later, the system displayed renewed activity that lasted through 2017 July. Here, we present radio and X-ray monitoring over ~3 months of the renewed activity to study the coupling between the jet and the inner regions of the disk/jet system. Our observations cover low X-ray luminosities that have not historically been well-sampled (LX~2×1033–1036 erg s–1; 1-10 keV), including time periods when the system was both brightening and fading. At these low luminosities, Swift J1753.5-0127 occupies a parameter space in the radio/X-ray luminosity plane that is comparable to "canonical" systems (e.g., GX 339-4), regardless of whether the system was brightening or fading, even though during its >=11 year outburst, Swift J1753.5-0127 emitted less radio emission from its jet than expected. We discuss implications for the existence of a single radio/X-ray luminosity correlation for black hole X-ray binaries at the lowest luminosities (LX 1035 erg s–1), and we compare to supermassive black holes. Our campaign includes the lowest luminosity quasi-simultaneous radio/X-ray detection to date for a black hole X-ray binary during its rise out of quiescence, thanks to early notification from optical monitoring combined with fast responses from sensitive multiwavelength facilities.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): stars: black holes - stars: individual: Swift J1753.5-0127 - X-rays: binaries - X-rays: binaries

Simbad objects: 13

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2021.06.14-03:07:49

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