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Cited by 1,439

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

On the fate of gas accreting at a low rate on to a black hole

Open access
Blandford, R. D., Begelman, M. C.·1999·Monthly Notices of the Royal Astronomical Society

Abstract

Gas supplied conservatively to a black hole at rates well below the Eddington rate may not be able to radiate effectively and the net energy flux, including the energy transported by the viscous torque, is likely to be close to zero at all radii. This has the consequence that the gas accretes with positive energy so that it may escape. Accordingly, we propose that only a small fraction of the gas supplied actually falls on to the black hole, and that the binding energy it releases is transported radially outward by the torque so as to drive away the remainder in the form of a wind. This is a generalization of and an alternative to an ‘ADAF’ solution. Some observational implications and possible ways to distinguish these two types of flow are briefly discussed.

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Crossref · 10.1046/j.1365-8711.1999.02358.x

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Metadata

Authors
Blandford, R. D., & Begelman, M. C.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1999-02-11
Volume
303
Issue
1
Pages
L1-L5
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2050444942
Cited by
1,439
References
1
FWCI
57.93
Type
journal article
Language
en
Open access
green

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Blandford, R. D., & Begelman, M. C. (1999). On the fate of gas accreting at a low rate on to a black hole. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.1999.02358.x

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.