Funnel stability and VLBI-jet luminosity

Details Funnel stability and VLBI-jet luminosity Funnel stability and VLBI-jet luminosity

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.222...37t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 222, Sept. 1, 1986, p. 37-47.

Astronomy and Astrophysics

Astronomy

Accretion Disks, Galactic Nuclei, Kelvin-Helmholtz Instability, Plasma Jets, Radio Jets (Astronomy), Very Long Base Interferometry, Kinetic Energy, Magnetohydrodynamic Stability, Optical Thickness

Scientific paper

The stability of the jet-funnel interface in thick disc models is investigated. In particular the authors analyse the circumstances in which the growth of Kelvin-Helmholtz instabilities can destroy the jet-funnel configuration, and the expected luminosity emitted at the top of the funnel from conversion of bulk kinetic energy into radiation via turbulent cascade processes.

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