Macroscopic currents and wind perturbations in the frame of the wind and shock model

Details Macroscopic currents and wind perturbations in the frame of the wind and shock model Macroscopic currents and wind perturbations in the frame of the wind and shock model

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xue..conf..215c&link_type=abstract

In Max-Planck Inst. für Physik und Astrophysik X-Ray and UV Emission from Active Galactic Nuclei p 215-217 (SEE N85-17790 08-88)

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Beam Currents, Galactic Nuclei, Magnetohydrodynamic Flow, Active Galactic Nuclei, Emission Spectra, Infrared Spectra, X Ray Spectra

Scientific paper

The formation of macroscopic currents in the shock layer of active galactic nuclei is analyzed. The results can be used to study the stability of the whole structure and to define a preferred direction in the formation of jets. Modifications caused by a perturbation in the wind to the IR-optical and X-ray regions of the emission spectrum are estimated.

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