Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6184
Title: Modelling of the spectral energy distribution of Fornax A: leptonic and hadronic production of high-energy emission from the radio lobes
Authors: McKinley, B.
Yang, R.
Deshpande, A.A.
Udaya Shankar, N.
Srivani, K.S.
Subrahmanyan, Ravi
+40 Co-authors
Keywords: active galaxies
NGC1316 radio continuum
Issue Date: 4-Feb-2015
Publisher: Oxford University Press for The Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 2015, Vol. 446, p3478-3491
Abstract: We present new low-frequency observations of the nearby radio galaxy Fornax A at 154 MHz with the Murchison Widefield Array, microwave flux-density measurements obtained from WMAP and Planck data, and γ-ray flux densities obtained from Fermi data. We also compile a comprehensive list of previously published images and flux-density measurements at radio, microwave and X-ray energies. A detailed analysis of the spectrum of Fornax A between 154 and 1510 MHz reveals that both radio lobes have a similar spatially averaged spectral index, and that there exists a steep-spectrum bridge of diffuse emission between the lobes. Taking the spectral index of both lobes to be the same, we model the spectral energy distribution of Fornax A across an energy range spanning 18 orders of magnitude, to investigate the origin of the X-ray and γ-ray emission. A standard leptonic model for the production of both the X-rays and γ-rays by inverse-Compton scattering does not fit the multiwavelength observations. Our results best support a scenario where the X-rays are produced by inverse-Compton scattering and the γ-rays are produced primarily by hadronic processes confined to the filamentary structures of the Fornax A lobes.
Description: Open Access
URI: http://hdl.handle.net/2289/6184
ISSN: 0035-8711
1365-2966 - (online)
Alternative Location: http://adsabs.harvard.edu/abs/2015MNRAS.446.3478M
http://arxiv.org/abs/1411.1487
http://dx.doi.org/10.1093/mnras/stu2310
Copyright: 2015 The authors & the Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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