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The inner jet of an active galactic nucleus as revealed by a radio-to-γ-ray outburst

Marscher, Alan P., Jorstad, Svetlana G., D'Arcangelo, Francesca D., Smith, Paul S., Williams, G. Grant, Larionov, Valeri M., Oh, Haruki, Olmstead, Alice R., Aller, Margo F., Aller, Hugh D., McHardy, Ian M., Lähteenmäki, Anne, Tornikoski, Merja, Valtaoja, Esko, Hagen-Thorn, Vladimir A., Kopatskaya, Eugenia N., Gear, Walter Kieran, Tosti, Gino, Kurtanidze, Omar, Nikolashvili, Maria, Sigua, Lorand, Miller, H. Richard and Ryle, Wesley T. 2008. The inner jet of an active galactic nucleus as revealed by a radio-to-γ-ray outburst. Nature 452 (7190) , pp. 966-969. 10.1038/nature06895

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Abstract

Blazars are the most extreme active galactic nuclei. They possess oppositely directed plasma jets emanating at near light speeds from accreting supermassive black holes. According to theoretical models, such jets are propelled by magnetic fields twisted by differential rotation of the black hole's accretion disk or inertial-frame-dragging ergosphere1, 2, 3. The flow velocity increases outward along the jet in an acceleration and collimation zone containing a coiled magnetic field4, 5. Detailed observations of outbursts of electromagnetic radiation, for which blazars are famous, can potentially probe the zone. It has hitherto not been possible to either specify the location of the outbursts or verify the general picture of jet formation. Here we report sequences of high-resolution radio images and optical polarization measurements of the blazar BL Lacertae. The data reveal a bright feature in the jet that causes a double flare of radiation from optical frequencies to TeV -ray energies, as well as a delayed outburst at radio wavelengths. We conclude that the event starts in a region with a helical magnetic field that we identify with the acceleration and collimation zone predicted by the theories. The feature brightens again when it crosses a standing shock wave corresponding to the bright 'core' seen on the images.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Physics and Astronomy
Publisher: Nature Publishing Group
ISSN: 0028-0836
Last Modified: 04 Jun 2017 01:59
URI: http://orca.cf.ac.uk/id/eprint/7288

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