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A self-similar model for extragalactic radio sources

Kaiser, C. R., Alexander, P.·1997·Monthly Notices of the Royal Astronomical Society

Abstract

An analytical model for extragalactic radio sources with pressure-confined jets is presented. We show that the properties of the bow shock and of the gas surrounding these objects force the sources to grow in a self-similar way provided the density in the external atmosphere falls less steeply than 1/d2. Results from observations and numerical simulations are used to develop a self-consistent model for the large-scale structure of FRII objects. The jets in these sources are shown to be stable against turbulence for the observed properties of FRIIs and the divide between FRI and FRII objects in jet power is reproduced. The overall dynamics of a source are derived as a function of time and depend on the external density, the jet power and the scaleheight of the external atmosphere. Derived dynamical ages are consistent with observed spectral ages.

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Metadata

Authors
Kaiser, C. R., & Alexander, P.
Venue
Monthly Notices of the Royal Astronomical Society
Published
1997-03-21
Volume
286
Issue
1
Pages
215-222
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2059075380
Cited by
453
References
0
FWCI
6.58
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: A self-similar model for extragalactic radio sources. https://app.cochat.ai/papers/10.1093/mnras/286.1.215
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Kaiser, C. R., & Alexander, P. (1997). A self-similar model for extragalactic radio sources. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/286.1.215

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.