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- W2022709442 abstract "There is mounting evidence that mechanical radio source feedback is important in galaxy evolution and in order to quantify this feedback, detailed models of radio source evolution are required. We present an extension to current analytic models that encompasses young radio sources with physical sizes on sub-kiloparsec scales. This work builds on an existing young source dynamical model to include radiative losses in a flat environment, and as such, is the best physically motivated compact symmetric object model to date. Results predict that young radio sources experience significant radiative loss on length-scales and spectral scales consistent with observed compact steep spectrum sources. We include full expressions for the transition to self-similar expansion and present this complete model of radio source evolution from first cocoon formation to end of source lifetime around 108 years within the context of a simplified King profile external atmosphere." @default.
- W2022709442 created "2016-06-24" @default.
- W2022709442 creator A5023638585 @default.
- W2022709442 creator A5072981488 @default.
- W2022709442 date "2014-07-02" @default.
- W2022709442 modified "2023-10-16" @default.
- W2022709442 title "Radio source evolution on galactic scales" @default.
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- W2022709442 doi "https://doi.org/10.1093/mnras/stu1111" @default.
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