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Numerical Observations of a Restarting Radio Jet
Published online by Cambridge University Press: 19 July 2016
Abstract
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An MHD computation of a restarting jet is presented and compared with observations of classical double radio sources. Assuming ideal MHD and an adiabatic equation of state, it is found that a “partial” jet exists for about 25% of the time, and that the terminal hotspot dissipates quickly compared to other physical time scales once the outflow of the jet is terminated.
- Type
- 8. The Role of Magnetic Fields in Radio Source Jets and Extended Radio Lobes
- Information
- Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 435 - 436
- Copyright
- Copyright © Kluwer 1990
References
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