Numerical simulations of bent, disrupted radio jets

Details Numerical simulations of bent, disrupted radio jets Numerical simulations of bent, disrupted radio jets

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..219l&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 219-220 (SEE N93-26706 10-90)

Computer Science

Numerical Analysis

1

Astronomical Models, Bending, Hydrodynamics, Intergalactic Media, Interstellar Matter, Numerical Analysis, Radio Jets (Astronomy), Supersonic Jet Flow, Three Dimensional Models, Crossings, Discontinuity, Wind Direction

Scientific paper

We present preliminary results from three-dimensional hydrodynamical simulations designed to investigate the physics of jet bending and disruption. The specific scenario considered here involves a mildly supersonic jet crossing a contact discontinuity at the interface between the interstellar medium (ISM) and the intercluster medium (ICM) and then encountering a cross-wind in the ICM. The resultant morphologies show many of the features observed in radio sources including jet flaring, bending, and extended tails.

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