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arxiv: astro-ph/9805025 · v1 · submitted 1998-05-04 · 🌌 astro-ph

Accretion Disc-Corona Models and X/gamma-ray Spectra of Accreting Black Holes

classification 🌌 astro-ph
keywords accretingaccretionblackdisc-coronagamma-rayholesmodelsproperties
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We discuss properties of thermal and hybrid (thermal/non-thermal) electron-positron plasmas in the pair and energy equilibria. Various accretion disc-corona models, recently proposed to explain properties of galactic as well as extragalactic accreting black holes, are confronted with the observed broad-band X-ray and gamma-ray spectra.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion

    astro-ph.HE 2026-05 unverdicted novelty 5.0

    Time lag analysis using ICCF on GX 339-4 data reveals state-dependent radio-X-ray delays interpreted as evidence for magnetic field transport linking the inner accretion flow and jet.