The Dynamics of Classical Double Radio Sources: Testing Self-Similar Models

Details The Dynamics of Classical Double Radio Sources: Testing Self-Similar Models The Dynamics of Classical Double Radio Sources: Testing Self-Similar Models

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cxo..prop..939h&link_type=abstract

Chandra Proposal ID #03700563

Physics

Chandra Proposal Id #03700563

Scientific paper

Although well-accepted models for the dynamics of classical double radio sources have been current for many years, it is only recently that they have progressed to the point at which they can be directly tested against observations. Kaiser (2000) has developed a model which predicts parameters of the hot-gas environment of well-behaved double sources from their observed radio spatial and spectral structure. We propose to test this model by observing the cluster environments of two intermediate-redshift radio sources. The observations will help to resolve important outstanding questions relating to the energy budget and particle content of these objects.

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