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A Wildly Flickering Jet in the Black Hole X-Ray Binary MAXI J1535-571

Cristina Baglio, Maria (author)
Istituto nazionale di astrofisica (INAF),New York University Abu Dhabi
Russell, David M. (author)
New York University Abu Dhabi
Casella, Piergiorgio (author)
Osservatorio Astronomico di Roma
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Al Noori, Hind (author)
New York University Abu Dhabi
Al Yazeedi, Aisha (author)
New York University Abu Dhabi
Belloni, Tomaso (author)
Istituto nazionale di astrofisica (INAF)
Buckley, David A.H. (author)
South African Astronomical Observatory
Cadolle Bel, Marion (author)
Ceccobello, Chiara, 1984 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Corbel, S. (author)
Institut de Recherche sur les Lois Fondamentales de l'Univers,Station de Radioastronomie de Nançay
Coti Zelati, Francesco (author)
Institut d'Estudis Espacials de Catalunya (IEEC),Institute of Space Studies of Catalonia (IEEC),Istituto nazionale di astrofisica (INAF),Universitat Autonoma de Barcelona (UAB)
Diaz-Trigo, M. (author)
European Southern Observatory (ESO)
Fender, R. P. (author)
University Of Oxford
Gallo, Elena (author)
University of Michigan
Gandhi, Poshak (author)
University of Southampton
Homan, Jeroen (author)
Netherlands Institute for Space Research (SRON),Eureka Scientific
Koljonen, Karri I.I. (author)
Aalto-Yliopisto,Aalto University,Turun Yliopisto,University of Turku
Lewis, Fraser (author)
Liverpool John Moores University,Cardiff University
Maccarone, T. J. (author)
Texas Tech University at Lubbock
Malzac, Julien (author)
Université de Toulouse,University of Toulouse
Markoff, S. (author)
Universiteit Van Amsterdam,University of Amsterdam
Miller-Jones, J. C. A. (author)
Curtin University
O'Brien, Kieran (author)
Durham University
Russell, Thomas D. (author)
Universiteit Van Amsterdam,University of Amsterdam
Saikia, P. (author)
New York University Abu Dhabi
Shahbaz, Tariq (author)
Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna
Sivakoff, G. R. (author)
University of Alberta
Soria, Roberto (author)
Curtin University,Chinese Academy of Sciences,The University of Sydney
Testa, Vincenzo (author)
Osservatorio Astronomico di Roma
Tetarenko, Alexandra J. (author)
University of Alberta,East Asian Observatory
Van Den Ancker, Mario E. (author)
European Southern Observatory (ESO)
Vincentelli, Federico M. (author)
Osservatorio Astronomico di Roma,Universita degli Studi dell'Insubria,University of Insubria,Istituto nazionale di astrofisica (INAF)
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 (creator_code:org_t)
2018-11-06
2018
English.
In: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 867:2
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We report on the results of optical, near-infrared (NIR), and mid-infrared observations of the black hole X-ray binary candidate (BHB) MAXI J1535-571 during its 2017/2018 outburst. During the first part of the outburst (MJD 58004-58012), the source shows an optical-NIR spectrum that is consistent with an optically thin synchrotron power law from a jet. After MJD 58015, however, the source faded considerably, the drop in flux being much more evident at lower frequencies. Before the fading, we measure a dereddened flux density of 100 mJy in the mid-infrared, making MAXI J1535-571 one of the brightest mid-infrared BHBs known so far. A significant softening of the X-ray spectrum is evident contemporaneous with the infrared fade. We interpret it as being due to the suppression of the jet emission, similar to the accretion-ejection coupling seen in other BHBs. However, MAXI J1535-571 did not transition smoothly to the soft state, instead showing X-ray hardness deviations associated with infrared flaring. We also present the first mid-IR variability study of a BHB on minute timescales, with a fractional rms variability of the light curves of ∼15%-22%, which is similar to that expected from the internal shock jet model, and much higher than the optical fractional rms (≲7%). These results represent an excellent case of multiwavelength jet spectral timing and demonstrate how rich, multiwavelength time-resolved data of X-ray binaries over accretion state transitions can help in refining models of the disk-jet connection and jet launching in these systems.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Annan fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Other Physics Topics (hsv//eng)

Keyword

accretion, accretion disks
ISM: jets and outflows
X-rays: binaries
black hole physics

Publication and Content Type

art (subject category)
ref (subject category)

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