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Nonthermal emission in radio galaxies from simulated relativistic electron transport in 3D MHD flows

Abstract:
We perform a series of so-called "synthetic observations" on a set of 3D MHD jet simulations which explicitly include energy-dependent transport of relativistic electrons, as described in the companion paper by Jones, Tregillis and Ryu. Analyzing them in light of the complex source dynamics and energetic particle distributions described in that paper, we find that the standard model for radiative aging in radio galaxies does not always adequately reflect the detailed source structure.
Publication status:
Published

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Journal:
PARTICLES AND FIELDS IN RADIO GALAXIES
Volume:
250
Pages:
336-339
Publication date:
2002-01-01
Event title:
Oxford Radio Galaxy Workshop
ISBN:
1583810900
Pubs id:
pubs:16030
UUID:
uuid:23a2f517-39a2-4140-8217-00afab168ec7
Local pid:
pubs:16030
Source identifiers:
16030
Deposit date:
2012-12-19

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