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Disk-Jet Coupling in the 2017/2018 Outburst of the Galactic Black Hole Candidate X-Ray Binary MAXI J1535-571

Russell, T. D. (author)
Universiteit Van Amsterdam,University of Amsterdam
Tetarenko, A. J. (author)
East Asian Observatory,University of Alberta
Miller-Jones, J. C. A. (author)
Curtin University
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Sivakoff, G. R. (author)
University of Alberta
Parikh, A. S. (author)
Universiteit Van Amsterdam,University of Amsterdam
Rapisarda, S. (author)
Chinese Academy of Sciences,Universiteit Van Amsterdam,University of Amsterdam
Wijnands, R. (author)
Universiteit Van Amsterdam,University of Amsterdam
Corbel, S. (author)
Université Paris-Saclay,University Paris-Saclay,Universite d'Orleans,University of Orléans
Tremou, E. (author)
Université Paris-Saclay,University Paris-Saclay
Altamirano, D. (author)
University of Southampton
Baglio, M. C. (author)
New York University Abu Dhabi
Ceccobello, Chiara, 1984 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Degenaar, N. (author)
Universiteit Van Amsterdam,University of Amsterdam
van den Eijnden, J. (author)
Universiteit Van Amsterdam,University of Amsterdam
Fender, R. (author)
University Of Oxford
Heywood, I (author)
Rhodes University,University Of Oxford
Krimm, H. A. (author)
National Science Foundation
Lucchini, M. (author)
Universiteit Van Amsterdam,University of Amsterdam
Markoff, S. (author)
Universiteit Van Amsterdam,University of Amsterdam
Russell, D. M. (author)
New York University Abu Dhabi
Soria, R. (author)
Chinese Academy of Sciences,The University of Sydney
Woudt, P. A. (author)
University of Cape Town
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 (creator_code:org_t)
2019-10-04
2019
English.
In: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 883:2
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • 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, 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 toward 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 = 0.69 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.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Annan fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Other Physics Topics (hsv//eng)
TEKNIK OCH TEKNOLOGIER  -- Elektroteknik och elektronik -- Signalbehandling (hsv//swe)
ENGINEERING AND TECHNOLOGY  -- Electrical Engineering, Electronic Engineering, Information Engineering -- Signal Processing (hsv//eng)

Keyword

black hole physics
ISM: jets and outflows
accretion, accretion disks
radio continuum: stars
X-rays: binaries
stars: individual (MAXI J1535-571)

Publication and Content Type

art (subject category)
ref (subject category)

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