# Extending the "Energetic Scaling of Relativistic Jets From Black Hole Systems" to Include $γ$-ray-loud X-ray Binaries

Lamb, GP and Kobayashi, S and Pian, E (2017) Extending the "Energetic Scaling of Relativistic Jets From Black Hole Systems" to Include $γ$-ray-loud X-ray Binaries. Monthly Notices of the Royal Astronomical Society, 472 (1). pp. 475-482. ISSN 0035-8711

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1705.09191v2.pdf - Accepted Version

We show that the jet power $P_j$ and geometrically corrected $\gamma$-ray luminosity $L_\gamma$ for the X-ray binaries (XRBs) Cygnus X-1, Cygnus X-3, and V404 Cygni, and $\gamma$-ray upper limits for GRS 1915+105 and GX339-4, follow the universal scaling for the energetics of relativistic jets from black hole (BH) systems found by Nemmen et al. (2012) for blazars and GRBs. The observed peak $\gamma$-ray luminosity for XRBs is geometrically corrected; and the minimum jet power is estimated from the peak flux density of radio flares and the flare rise time. The $L_\gamma-P_j$ correlation holds across $\sim 17$ orders of magnitude. The correlation suggests a jet origin for the high energy emission from X-ray binaries, and indicates a common mechanism or efficiency for the high energy emission 0.1-100 GeV from all relativistic BH systems.