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Advection-Dominated Accretion around Black Holes

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arxiv astro-ph/9803141 v1 pith:OZRXVW22 submitted 1998-03-12 astro-ph gr-qc

Ramesh Narayan , Rohan Mahadevan , Eliot Quataert (Harvard) This is my paper · ORCID
classification astro-phgr-qc
keywords blackaccretionadafsadvection-dominatedholesapplicationsaroundarticle
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This article reviews the physics of advection-dominated accretion flows (ADAFs) and describes applications to several black hole X-ray binaries and galactic nuclei. The possibility of using ADAFs to explore the event horizons of black holes is highlighted.

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Cited by 7 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 46 citations worldwide. Full citation record

  1. Thermal Conduction and Thermal-Driven Winds in Magnetized Viscous Accretion Disk Dynamics

    astro-ph.HE 2025-01 conditional novelty 7.0 of 10

    In a magnetized viscous accretion disk model, adding saturated thermal conduction and thermal-driven winds moves the standing shock outward from the black hole and shrinks the parameter space for shock solutions, offe...

  2. G objects as Primordial Black Hole-Neutron Star Remnants: Population Modeling and Multi-Wavelength Observables

    astro-ph.HE 2026-03 unverdicted novelty 6.0 of 10

    G objects are modeled as primordial black hole-neutron star remnants whose population simultaneously accounts for the Galactic Center pulsar deficit.

  3. The peculiar hard state behaviour of the black hole X-ray binary Swift J1727.8$-$1613

    astro-ph.HE 2025-06 conditional novelty 6.0 of 10

    In its 2023-2024 outburst, the black hole binary Swift J1727.8-1613 showed one of the most radio-quiet radio-X-ray tracks known, with X-ray spectral softening beginning just as the track changed slope.

  4. A New Interpretation for the Hot Corona in Active Galactic Nuclei

    astro-ph.HE 2025-02 conditional novelty 6.0 of 10

    The hot corona of an AGN is reinterpreted as a plasmoid chain in a parabolic reconnection layer, whose height tracks X-ray luminosity in a way that resembles IRAS 13224-3809 once a magnetic parameter is fitted.

  5. Radio Core Size of Low-luminosity Active Galactic Nuclei under the MAD-jet model

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    A MAD+jet model reproduces the observed ν^{-1} radio core-size scaling of LLAGNs only if jet electrons are mostly non-thermal, and predicts strong suppression of power-law electrons in MADs above L/L_Edd ≈ 3–8×10^{-6}.

  6. 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 of 10

    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.

  7. The physical mechanism of radio-quiet turn-on changing-look active galactic nuclei

    astro-ph.GA 2025-07 conditional novelty 5.0 of 10

    For most of 102 turn-on changing-look AGNs, the computed ADAF cooling timescale is shorter than the observed turn-on interval, which the authors take as support for an ADAF-collapse mechanism.

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