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A new lepto-hadronic model applied to the first simultaneous multiwavelength data set for Cygnus X-1

Kantzas, D. (author)
Universiteit Van Amsterdam,University of Amsterdam
Markoff, S. (author)
Universiteit Van Amsterdam,University of Amsterdam
Beuchert, T. (author)
Universiteit Van Amsterdam,University of Amsterdam,European Southern Observatory (ESO)
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Lucchini, M. (author)
Universiteit Van Amsterdam,University of Amsterdam
Chhotray, A. (author)
Universiteit Van Amsterdam,University of Amsterdam
Ceccobello, Chiara, 1984 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Tetarenko, Alexandra J. (author)
East Asian Observatory
Miller-Jones, J. C. A. (author)
Curtin University
Bremer, M. (author)
Institut de Radioastronomie Millimétrique (IRAM)
Garcia, J. A. (author)
California Institute of Technology (Caltech)
Grinberg, V. (author)
Eberhard Karls Universität Tübingen,Eberhard Karls University of Tübingen
Uttley, P. (author)
Universiteit Van Amsterdam,University of Amsterdam
Wilms, J. (author)
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 (creator_code:org_t)
2020-10-29
2020
English.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 500:2, s. 2112-2126
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Cygnus X-1 is the first Galactic source confirmed to host an accreting black hole. It has been detected across the entire electromagnetic spectrum from radio to GeV gamma-rays. The source's radio through mid-infrared radiation is thought to originate from the relativistic jets. The observed high degree of linear polarization in the MeV X-rays suggests that the relativistic jets dominate in this regime as well, whereas a hot accretion flow dominates the soft X-ray band. The origin of the GeV non-thermal emission is still debated, with both leptonic and hadronic scenarios deemed to be viable. In this work, we present results from a new semi-analytical, multizone jet model applied to the broad-band spectral energy distribution of Cygnus X-1 for both leptonic and hadronic scenarios. We try to break this degeneracy by fitting the first-ever high-quality, simultaneous multiwavelength data set obtained from the CHOCBOX campaign (Cygnus X-1 Hard state Observations of a Complete Binary Orbit in X-rays). Our model parametrizes dynamical properties, such as the jet velocity profile, the magnetic field, and the energy density. Moreover, the model combines these dynamical properties with a self-consistent radiative transfer calculation including secondary cascades, both of leptonic and hadronic origin. We conclude that sensitive TeV gamma-ray telescopes like Cherenkov Telescope Array (CTA) will definitively answer the question of whether hadronic processes occur inside the relativistic jets of Cygnus X-1.

Subject headings

NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

X-rays: individual: Cyg X-1
acceleration of particles
radiation mechanisms: non-thermal

Publication and Content Type

art (subject category)
ref (subject category)

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