SIMBAD references

2017MNRAS.472..475L - Mon. Not. R. Astron. Soc., 472, 475-482 (2017/November-3)

Extending the 'energetic scaling of relativistic jets from black hole systems' to include γ-ray-loud X-ray binaries.

LAMB G.P., KOBAYASHI S. and PIAN E.

Abstract (from CDS):

We show that the jet power Pj and geometrically corrected γ-ray luminosity Lγ for the X-ray binaries (XRBs) Cygnus X-1, Cygnus X-3, and V404 Cygni, and γ-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. for blazars and GRBs. The observed peak γ-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 Lγ-Pj correlation holds across ∼17 orders of magnitude. The correlation suggests a jet origin for the high-energy emission from XRBs, and indicates a common mechanism or efficiency for the high-energy emission 0.1-100 GeV from all relativistic BH systems.

Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): relativistic processes - stars: jets - X-rays: binaries

Simbad objects: 10

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2021.06.25-16:28:32

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