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Jet–Accretion System in the Nearby mJy Radio Galaxies

  • Authors: Paola Grandi, Eleonora Torresi, Duccio Macconi, Bia Boccardi, and Alessandro Capetti

2021 The Astrophysical Journal 911 17.

  • Provider: AAS Journals

Caption: Figure 5.

Left panel—[η/ϵf] parameter space for FRIs, FRII-LERGs and FRII-HERGs with z > 0.05. The curves are obtained via Equation (2) by assuming the average L[O III] and LNVSS luminosities (and standard deviation σ) in Table 2. Dotted lines correspond to 1σ uncertainty. The separation at ﹩\mathrm{Log}({L}_{[{\rm{O}}{\rm\small{III}}]}/{L}_{\mathrm{Edd}})=-6.7﹩ between HERGs and LERGs is based on Figure 4. The intersections of the horizontal line with the curves mark the f values required to have the same efficiency ratio (η/ϵ = 0.98 in this case) in each class. Right panel—same plot for FR0s, small FRIs, and FRIs with z ≤ 0.05. The horizontal line corresponds to η/ϵ = 0.49. The vertical arrows indicate that the η/ϵ values traced by the curves have to be intended as upper limits.

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