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Numerical Simulations of Extragalactic Jets in an Inhomogeneous Environment
Published online by Cambridge University Press: 25 May 2016
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We have simulated the passage of an extragalactic jet through a medium containing an ensemble of cool, dense clouds. The hydrodynamic code uses the second-order Godunov method of Falle (Falle 1991, van Leer 1979) in three-dimensional, cartesian coordinates. We have estimated the synchrotron emissivity and used this to produce synthetic radio maps. The results are reminiscent of structures seen in many extragalactic radio sources.
- Type
- Radio Source Modelling and Emission Mechanisms
- Information
- Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 467 - 468
- Copyright
- Copyright © Kluwer 1996
References
Higgins, et al., (1995) In:
‘Shocks in Astrophysics’
, eds. Millar, T.J. & Raga, A., in press.Google Scholar
Wilson, A. S. (1993) In:
‘Astrophysical Jets’
, STScI Symp. Ser. Vol. 6, eds. Burgarella, , Livio & O'Dea, pp.122
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