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

Kantzas, D. and Markoff, S. and Beuchert, T. and Lucchini, M. and Chhotray, A. and Ceccobello, C. and Tetarenko, A. J. and Miller-Jones, J. C. A. and Bremer, M. and García, J. A. and Grinberg, V. and Uttley, P. and Wilms, J. (2021) A new lepto-hadronic model applied to the first simultaneous multiwavelength data set for Cygnus X–1. Monthly Notices of the Royal Astronomical Society, 500 (2). pp. 2112-2126. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20210209-120605988

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Abstract

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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/staa3349DOIArticle
https://arxiv.org/abs/2010.08501arXivDiscussion Paper
https://dx.doi.org/10.5281/zenodo.4126910DOIData
ORCID:
AuthorORCID
Kantzas, D.0000-0002-7364-606X
Markoff, S.0000-0001-9564-0876
Lucchini, M.0000-0002-2235-3347
Ceccobello, C.0000-0002-4767-9925
Tetarenko, A. J.0000-0003-3906-4354
Miller-Jones, J. C. A.0000-0003-3124-2814
García, J. A.0000-0003-3828-2448
Grinberg, V.0000-0003-2538-0188
Uttley, P.0000-0001-9355-961X
Wilms, J.0000-0003-2065-5410
Additional Information:© 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2020 October 20. Received 2020 October 16; in original form 2020 March 3. Published: 29 October 2020. We would like to thank the reviewer for the very helpful comments on improving the original manuscript. DK would like to thank Maria Petropoulou for fruitful discussions, and Ping Zhou and Thomas Russell for useful comments on the manuscript. DK, SM, ML, and AC were supported by the Netherlands Organisation for Scientific Research (NWO) VICI grant (no. 639.043.513). VG is supported through the Margarete von Wrangell fellowship by the ESF and the Ministry of Science, Research and the Arts Baden-Württemberg. JCAM-J is the recipient of an Australian Research Council Future Fellowship (FT140101082), funded by the Australian government. This work is based on observations carried out under the project number W15BQ with the IRAM NOEMA Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain). This research made use of ASTROPY (http://www.astropy.org) a community-developed core PYTHON package for Astronomy (Astropy Collaboration et al. 2013; Price-Whelan et al. 2018), MATPLOTLIB (Hunter 2007), NUMPY (Oliphant 2006), SCIPY (Virtanen et al. 2020), ISIS functions (ISISscripts) provided by ECAP/Remeis observatory and MIT (http://www.sternwarte.unierlangen.de/isis/), and the CTA instrument response functions provided by the CTA Consortium and Observatory, see http://www.cta-observatory.org/science/cta-performance/ (version prod3b-v2) for more details. Data Availability: The data underlying this article are available in Zenodo, at https://dx.doi.org/10.5281/zenodo.4126910.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)639.043.513
European Social FundUNSPECIFIED
Ministry of Science, Research and the Arts (Baden-Württemberg)UNSPECIFIED
Australian Research CouncilFT140101082
Subject Keywords:acceleration of particles – radiation mechanisms: non-thermal – X-rays: individual: Cyg X–1
Issue or Number:2
Record Number:CaltechAUTHORS:20210209-120605988
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210209-120605988
Official Citation:D Kantzas, S Markoff, T Beuchert, M Lucchini, A Chhotray, C Ceccobello, A J Tetarenko, J C A Miller-Jones, M Bremer, J A Garcia, V Grinberg, P Uttley, J Wilms, A new lepto-hadronic model applied to the first simultaneous multiwavelength data set for Cygnus X–1, Monthly Notices of the Royal Astronomical Society, Volume 500, Issue 2, January 2021, Pages 2112–2126, https://doi.org/10.1093/mnras/staa3349
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:107966
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Feb 2021 21:11
Last Modified:09 Feb 2021 21:12

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