Ambient effects on astrophysical jets

Details Ambient effects on astrophysical jets Ambient effects on astrophysical jets

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spub.rept.....d&link_type=abstract

Conference Paper, Sao Paulo Univ. Brazil Inst. Astronomico e Geofisico.

Astronomy and Astrophysics

Astronomy

Radio Jets (Astronomy), Supersonic Flow, Three Dimensional Models, Hydrodynamic Equations, Ambience, Pressure Gradients, Computerized Simulation, Stratified Flow, Flow Distribution, Radiant Cooling, Helmholtz Vorticity Equation, Shock Waves

Scientific paper

Supersonic jets are produced by Young Stars and Active Nuclei of Galaxies and propagate over large scales into a surrounding medium which is, in general, non-homogeneous. Previous 3-D numerical simulations were performed for jets propagating solely in homogeneous ambient media. We here present fully 3-D hydrodynamical simulations of jets propagating in more realistic atmospheres containing positive and negative pressure and density gradients.

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