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Cited by 331

The DOI matches its Crossref record; 6 of the 6 references it cites were found in a registry or an index.

A change in the optical polarization associated with a γ-ray flare in the blazar 3C 279

Open access
The Fermi-LAT Collaboration and members of the 3C 279 multi-band campaign·2010·Nature

Abstract

It is widely accepted that strong and variable radiation detected over all accessible energy bands in a number of active galaxies arises from a relativistic, Doppler-boosted jet pointing close to our line of sight. The size of the emitting zone and the location of this region relative to the central supermassive black hole are, however, poorly known, with estimates ranging from light-hours to a light-year or more. Here we report the coincidence of a gamma (γ)-ray flare with a dramatic change of optical polarization angle. This provides evidence for co-spatiality of optical and γ-ray emission regions and indicates a highly ordered jet magnetic field. The results also require a non-axisymmetric structure of the emission zone, implying a curved trajectory for the emitting material within the jet, with the dissipation region located at a considerable distance from the black hole, at about 105 gravitational radii.

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Crossref · 10.1038/nature08841

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Metadata

Authors
The Fermi-LAT Collaboration and members of the 3C 279 multi-band campaign
Venue
Nature
Published
2010-02
Volume
463
Issue
7283
Pages
919-923
ISSN
  • 0028-0836 (ISSN-L)
  • 1476-4687
OpenAlex
W2119367243
Cited by
331
References
6
FWCI
18.71
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: A change in the optical polarization associated with a γ-ray flare in the blazar 3C 279. https://app.cochat.ai/papers/10.1038/nature08841
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The Fermi-LAT Collaboration and members of the 3C 279 multi-band campaign. (2010). A change in the optical polarization associated with a γ-ray flare in the blazar 3C 279. Nature. https://doi.org/10.1038/nature08841

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

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