A new lepto-hadronic model applied to the first simultaneous multiwavelength data set for Cygnus X-1
Artikel i vetenskaplig tidskrift, 2020
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.
X-rays: individual: Cyg X-1
acceleration of particles
radiation mechanisms: non-thermal
Författare
D. Kantzas
Universiteit Van Amsterdam
S. Markoff
Universiteit Van Amsterdam
T. Beuchert
Universiteit Van Amsterdam
European Southern Observatory (ESO)
M. Lucchini
Universiteit Van Amsterdam
A. Chhotray
Universiteit Van Amsterdam
Chiara Ceccobello
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Alexandra J. Tetarenko
East Asian Observatory
J. C. A. Miller-Jones
Curtin University
M. Bremer
Institut de Radioastronomie Millimétrique (IRAM)
J. A. Garcia
California Institute of Technology (Caltech)
Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics
V. Grinberg
Universität Tübingen
P. Uttley
Universiteit Van Amsterdam
J. Wilms
Dr. Karl Remeis-Observatory and Erlangen Centre for Astroparticle Physics
Monthly Notices of the Royal Astronomical Society
0035-8711 (ISSN) 1365-2966 (eISSN)
Vol. 500 2 2112-2126Ämneskategorier (SSIF 2011)
Subatomär fysik
Astronomi, astrofysik och kosmologi
DOI
10.1093/mnras/staa3349
Relaterade dataset
A new lepto-hadronic model applied to the first simultaneous multiwavelength data set for Cygnus X–1 [dataset]
DOI: 10.5281/zenodo.4126909