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Cited by 413

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

Poynting Jets from Black Holes and Cosmological Gamma-Ray Bursts

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Mészáros, P., Rees, M. J.·1997·The Astrophysical Journal

Abstract

We discuss the properties of magnetically dominated jetlike outflows from stellar mass black holes surrounded by debris tori resulting from neutron star disruption. These jets may have narrow cores (along the rotation axis) that are almost free of baryons and attain very high bulk Lorentz factors ≳10 6 . The jets give rise to a characteristic MeV to TeV emission as well as to relativistic shocks producing the usual MeV bursts. Because the outflow is highly directional, the properties of the observed gamma rays would depend on the viewing angle relative to the rotation axis. Even for the most intense bursts, which under the assumption of isotropic emission and substantial redshifts would be inferred to emit 10 52 -10 53 ergs, the efficiencies required are only 10 -2 to 10 -4 .

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Metadata

Authors
Mészáros, P., & Rees, M. J.
Venue
The Astrophysical Journal
Published
1997-06-10
Volume
482
Issue
1
Pages
L29-L32
ISSN
0004-637X (ISSN-L)
OpenAlex
W1999798892
Cited by
413
References
1
FWCI
20.07
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Poynting Jets from Black Holes and Cosmological Gamma-Ray Bursts. https://app.cochat.ai/papers/10.1086/310692
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Mészáros, P., & Rees, M. J. (1997). Poynting Jets from Black Holes and Cosmological Gamma-Ray Bursts. The Astrophysical Journal. https://doi.org/10.1086/310692

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