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Cited by 434

The DOI matches its Crossref record; 12 of the 12 references it cites were found in a registry or an index.

Convection‐dominated Accretion Flows

Open access
Quataert, Eliot, Gruzinov, Andrei·2000·The Astrophysical Journal

Abstract

Nonradiating advection-dominated accretion flows are convectively unstable in the radial direction. We calculate the two-dimensional ( r -θ) structure of such flows assuming that (1) convection transports angular momentum inward, opposite to normal viscosity, and (2) viscous transport by other mechanisms (e.g., magnetic fields) is weak (α ≪ 1). Under such conditions convection dominates the dynamics of the accretion flow and leads to a steady state structure that is marginally stable to convection. We show that the marginally stable flow has a constant temperature and rotational velocity on spherical shells, a net flux of energy from small to large radii, zero net accretion rate, and a radial density profile of ρ ∝ r -1/2 , flatter than the ρ ∝ r -3/2 profile characteristic of spherical accretion flows. This solution accurately describes the full two-dimensional structure of recent axisymmetric numerical simulations of advection-dominated accretion flows.

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Metadata

Authors
Quataert, E., & Gruzinov, A.
Venue
The Astrophysical Journal
Published
2000-08-20
Volume
539
Issue
2
Pages
809-814
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1990558603
Cited by
434
References
12
FWCI
22.97
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Convection‐dominated Accretion Flows. https://app.cochat.ai/papers/10.1086/309267
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Quataert, E., & Gruzinov, A. (2000). Convection‐dominated Accretion Flows. The Astrophysical Journal. https://doi.org/10.1086/309267

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