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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
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 5 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. 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.

  2. 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.

  3. 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}.

  4. 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.

  5. 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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