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Is the core of M87 the source of its TeV emission? Implications for unified schemes

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arxiv astro-ph/0510783 v1 pith:AMHYXA23 submitted 2005-10-27 astro-ph

classification astro-ph
keywords coreemissionsourcecomptonenergyfailflowflux
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M87 has been recently shown to be a TeV source which is likely to be variable. Based on this, and on contemporaneous optical and X-ray monitoring, we argue that the source of the TeV emission is the core of M87 and not one of two jet knots (HST-1 and A) with X-ray brightness comparable to that of the core. We model the TeV emission in the core as inverse Compton (IC) emission from the base of the jet. Homogeneous models fail to reproduce the spectral energy distribution (SED) and, in particular, the TeV flux. They also fail to comply with the unified scheme of BL Lacertae (BL) objects and FR I radio galaxies. A jet that decelerates from a Lorentz factor Gamma ~ 20 down to Gamma \~ 5 over a length of ~ 0.1 pc reproduces the observed SED of the M87 core, and, when aligned to the line of sight, produces a SED similar to those of TeV BLs. The TeV flux in the decelerating jet model is successfully reproduced as upstream Compton (UC) scattering, a recently identified emission mechanism, in which energetic electrons of the upstream faster flow upscatter the low energy photons produced in the slower downstream part of the flow.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 72 citations worldwide. Full citation record

  1. Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars

    astro-ph.HE 2026-07 accept novelty 6.0 of 10

    Systematic Fermi-LAT search detects VHE emission from 14 Compton-dominated blazars (4 new at >5σ) and constrains the emitting region to >1.1–1.4 BLR radii.

  2. M87: a cosmic laboratory for deciphering black hole accretion and jet formation

    astro-ph.HE 2024-12 unverdicted novelty 1.0 of 10

    A comprehensive review of M87's black hole, accretion flow, and jet observations from event-horizon to kiloparsec scales, with no new measurements.

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