Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-30T07:42:06.361Z Has data issue: false hasContentIssue false

Analytical Modelling of Linear Size Evolution of Powerful Radio Sources

Published online by Cambridge University Press:  25 May 2016

Krzysztof T. Chyży*
Affiliation:
Astronomical Observatory of the Jagiellonian University ul. Orla 171, 30-244 Kraków, Poland

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We assume that two continuous, supersonic jets of plasma advance into a uniform surrounding medium of constant density and pressure. In terms of fluid dynamics their propagation is described by the kinetic model suitable for high Mach number flows, which likely occur in edge-brightened powerful radio sources. In this approximation the jet flowing energy is dominated by the bulk energy of thermal material. The end of the jet enters the undisturbed ambient medium and forms a front shock, where the supplied bulk energy is in situ transferred to relativistic particles and magnetic field.

Type
Radio Source Modelling and Emission Mechanisms
Copyright
Copyright © Kluwer 1996 

References

Chyży, K.T., Zieba, S. (1995) A&A , 303, 420 Google Scholar
Eilek, J.A., Shore, S.N., 1989 ApJ 342, 187 Google Scholar
Hardee, P.E., White, R.W., Norman, M.L., Cooper, M.A., Clarke, D.A., 1992 ApJ , 387, 460 Google Scholar