Viscous jets

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Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.207..255n&link_type=abstract

In ESA Plasma Astrophys. p 255-257 (SEE N85-22270 12-90)

Astronomy and Astrophysics

Astrophysics

Galactic Nuclei, Gas Dynamics, Gas Viscosity, Plasma Jets, Active Galaxies, Astronomical Models, Entrainment, Plasma Turbulence

Scientific paper

The starting flow is calculated around an object representing a central
engine of an active galaxy that imparts momentum unidirectionally to its
surroundings. Viscosity is used to mimic turbulence. A steady jet
results for which the rate of entrainment of gas can be numerically
computed. Comparison is made with analytical calculations.

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