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On the Radial Structure of Radiatively Inefficient Accretion Flows with Convection

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arxiv astro-ph/0110371 v1 pith:26CK2PGH submitted 2001-10-16 astro-ph

Marek A. Abramowicz , Igor V.Igumenshchev , Eliot Quataert , Ramesh Narayan This is my paper · ORCID
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We consider the radial structure of radiatively inefficient hydrodynamic accretion flows around black holes. We show that low-viscosity flows consist of two zones: an outer convection-dominated zone and an inner advection-dominated zone. The transition between these two zones occurs at ~50 Schwarzschild radii.

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  1. 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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