Modelling of the spectral energy distribution of fornax A

Leptonic and hadronic production of high-energy emission from the radio lobes

B. McKinley, R. Yang, M. López-Caniego, F. Briggs, N. Hurley-Walker, R. B. Wayth, A. R. Offringa, R. Crocker, G. Bernardi, P. Procopio, B. M. Gaensler, S. J. Tingay, M. Johnston-Hollitt, M. McDonald, M. Bell, N. D R Bhat, Judd Bowman, R. J. Cappallo, B. E. Corey, A. A. Deshpande & 35 others D. Emrich, A. Ewall-Wice, L. Feng, R. Goeke, L. J. Greenhill, B. J. Hazelton, J. N. Hewitt, L. Hindson, Daniel Jacobs, D. L. Kaplan, J. C. Kasper, E. Kratzenberg, N. Kudryavtseva, E. Lenc, C. J. Lonsdale, M. J. Lynch, S. R. McWhirter, D. A. Mitchell, M. F. Morales, E. Morgan, D. Oberoi, S. M. Ord, B. Pindor, T. Prabu, J. Riding, A. E E Rogers, D. A. Roshi, N. Udaya Shankar, K. S. Srivani, R. Subrahmanyan, M. Waterson, R. L. Webster, A. R. Whitney, A. Williams, C. L. Williams

Research output: Contribution to journalArticle

16 Citations (Scopus)

Abstract

We present new low-frequency observations of the nearby radio galaxy Fornax A at 154MHz 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 1510MHz 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.

Original languageEnglish (US)
Pages (from-to)3478-3491
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume446
Issue number4
DOIs
StatePublished - 2014

Fingerprint

spectral energy distribution
lobes
rays
radio
flux density
modeling
energy
x rays
scattering
microwaves
radio galaxies
lists
low frequencies
distribution
index
microwave

Keywords

  • Galaxies: active
  • Galaxies: individual: NGC1316
  • Radio continuum: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Modelling of the spectral energy distribution of fornax A : Leptonic and hadronic production of high-energy emission from the radio lobes. / McKinley, B.; Yang, R.; López-Caniego, M.; Briggs, F.; Hurley-Walker, N.; Wayth, R. B.; Offringa, A. R.; Crocker, R.; Bernardi, G.; Procopio, P.; Gaensler, B. M.; Tingay, S. J.; Johnston-Hollitt, M.; McDonald, M.; Bell, M.; Bhat, N. D R; Bowman, Judd; Cappallo, R. J.; Corey, B. E.; Deshpande, A. A.; Emrich, D.; Ewall-Wice, A.; Feng, L.; Goeke, R.; Greenhill, L. J.; Hazelton, B. J.; Hewitt, J. N.; Hindson, L.; Jacobs, Daniel; Kaplan, D. L.; Kasper, J. C.; Kratzenberg, E.; Kudryavtseva, N.; Lenc, E.; Lonsdale, C. J.; Lynch, M. J.; McWhirter, S. R.; Mitchell, D. A.; Morales, M. F.; Morgan, E.; Oberoi, D.; Ord, S. M.; Pindor, B.; Prabu, T.; Riding, J.; Rogers, A. E E; Roshi, D. A.; Udaya Shankar, N.; Srivani, K. S.; Subrahmanyan, R.; Waterson, M.; Webster, R. L.; Whitney, A. R.; Williams, A.; Williams, C. L.

In: Monthly Notices of the Royal Astronomical Society, Vol. 446, No. 4, 2014, p. 3478-3491.

Research output: Contribution to journalArticle

McKinley, B, Yang, R, López-Caniego, M, Briggs, F, Hurley-Walker, N, Wayth, RB, Offringa, AR, Crocker, R, Bernardi, G, Procopio, P, Gaensler, BM, Tingay, SJ, Johnston-Hollitt, M, McDonald, M, Bell, M, Bhat, NDR, Bowman, J, Cappallo, RJ, Corey, BE, Deshpande, AA, Emrich, D, Ewall-Wice, A, Feng, L, Goeke, R, Greenhill, LJ, Hazelton, BJ, Hewitt, JN, Hindson, L, Jacobs, D, Kaplan, DL, Kasper, JC, Kratzenberg, E, Kudryavtseva, N, Lenc, E, Lonsdale, CJ, Lynch, MJ, McWhirter, SR, Mitchell, DA, Morales, MF, Morgan, E, Oberoi, D, Ord, SM, Pindor, B, Prabu, T, Riding, J, Rogers, AEE, Roshi, DA, Udaya Shankar, N, Srivani, KS, Subrahmanyan, R, Waterson, M, Webster, RL, Whitney, AR, Williams, A & Williams, CL 2014, 'Modelling of the spectral energy distribution of fornax A: Leptonic and hadronic production of high-energy emission from the radio lobes', Monthly Notices of the Royal Astronomical Society, vol. 446, no. 4, pp. 3478-3491. https://doi.org/10.1093/mnras/stu2310
McKinley, B. ; Yang, R. ; López-Caniego, M. ; Briggs, F. ; Hurley-Walker, N. ; Wayth, R. B. ; Offringa, A. R. ; Crocker, R. ; Bernardi, G. ; Procopio, P. ; Gaensler, B. M. ; Tingay, S. J. ; Johnston-Hollitt, M. ; McDonald, M. ; Bell, M. ; Bhat, N. D R ; Bowman, Judd ; Cappallo, R. J. ; Corey, B. E. ; Deshpande, A. A. ; Emrich, D. ; Ewall-Wice, A. ; Feng, L. ; Goeke, R. ; Greenhill, L. J. ; Hazelton, B. J. ; Hewitt, J. N. ; Hindson, L. ; Jacobs, Daniel ; Kaplan, D. L. ; Kasper, J. C. ; Kratzenberg, E. ; Kudryavtseva, N. ; Lenc, E. ; Lonsdale, C. J. ; Lynch, M. J. ; McWhirter, S. R. ; Mitchell, D. A. ; Morales, M. F. ; Morgan, E. ; Oberoi, D. ; Ord, S. M. ; Pindor, B. ; Prabu, T. ; Riding, J. ; Rogers, A. E E ; Roshi, D. A. ; Udaya Shankar, N. ; Srivani, K. S. ; Subrahmanyan, R. ; Waterson, M. ; Webster, R. L. ; Whitney, A. R. ; Williams, A. ; Williams, C. L. / Modelling of the spectral energy distribution of fornax A : Leptonic and hadronic production of high-energy emission from the radio lobes. In: Monthly Notices of the Royal Astronomical Society. 2014 ; Vol. 446, No. 4. pp. 3478-3491.
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abstract = "We present new low-frequency observations of the nearby radio galaxy Fornax A at 154MHz 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 1510MHz 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.",
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TY - JOUR

T1 - Modelling of the spectral energy distribution of fornax A

T2 - Leptonic and hadronic production of high-energy emission from the radio lobes

AU - McKinley, B.

AU - Yang, R.

AU - López-Caniego, M.

AU - Briggs, F.

AU - Hurley-Walker, N.

AU - Wayth, R. B.

AU - Offringa, A. R.

AU - Crocker, R.

AU - Bernardi, G.

AU - Procopio, P.

AU - Gaensler, B. M.

AU - Tingay, S. J.

AU - Johnston-Hollitt, M.

AU - McDonald, M.

AU - Bell, M.

AU - Bhat, N. D R

AU - Bowman, Judd

AU - Cappallo, R. J.

AU - Corey, B. E.

AU - Deshpande, A. A.

AU - Emrich, D.

AU - Ewall-Wice, A.

AU - Feng, L.

AU - Goeke, R.

AU - Greenhill, L. J.

AU - Hazelton, B. J.

AU - Hewitt, J. N.

AU - Hindson, L.

AU - Jacobs, Daniel

AU - Kaplan, D. L.

AU - Kasper, J. C.

AU - Kratzenberg, E.

AU - Kudryavtseva, N.

AU - Lenc, E.

AU - Lonsdale, C. J.

AU - Lynch, M. J.

AU - McWhirter, S. R.

AU - Mitchell, D. A.

AU - Morales, M. F.

AU - Morgan, E.

AU - Oberoi, D.

AU - Ord, S. M.

AU - Pindor, B.

AU - Prabu, T.

AU - Riding, J.

AU - Rogers, A. E E

AU - Roshi, D. A.

AU - Udaya Shankar, N.

AU - Srivani, K. S.

AU - Subrahmanyan, R.

AU - Waterson, M.

AU - Webster, R. L.

AU - Whitney, A. R.

AU - Williams, A.

AU - Williams, C. L.

PY - 2014

Y1 - 2014

N2 - We present new low-frequency observations of the nearby radio galaxy Fornax A at 154MHz 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 1510MHz 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.

AB - We present new low-frequency observations of the nearby radio galaxy Fornax A at 154MHz 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 1510MHz 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.

KW - Galaxies: active

KW - Galaxies: individual: NGC1316

KW - Radio continuum: galaxies

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U2 - 10.1093/mnras/stu2310

DO - 10.1093/mnras/stu2310

M3 - Article

VL - 446

SP - 3478

EP - 3491

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -