Relativistic jet simulations

Details Relativistic jet simulations Relativistic jet simulations

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..373b&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 373-374

Astronomy and Astrophysics

Astrophysics

Adiabatic Conditions, Astronomical Models, Cooling Flows (Astrophysics), Radio Jets (Astronomy), Relativistic Plasmas, Axisymmetric Flow, Magnetohydrodynamic Flow, Shock Waves, Simulation, Steady State

Scientific paper

Observations on parsec scales suggest that the flow in extragalactic
radio sources has both bulk and thermal Lorentz factors which are
significantly greater than one. An axisymmetric jet was simulated using
Godunov's method to solve the transformed equations in the steady state
case. A brief description of the simulation results is presented.

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