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arXiv · 1912.05527

On the Radio Image of Relativistic Jets -- I. Internal Structure, Doppler Boosting, and Polarization Maps

A. V. Chernoglazov·V. S. Beskin·V. I. Pariev
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Abstract

In this first paper from forthcoming series of works devoted to radio image of relativistic jets from active galactic nuclei the role of internal structure of a flow is discussed. We determine the radial profiles of all physical values for reasonable Michel magnetization parameter $\sigma_{\rm M}$ and ambient pressure $P_{\rm ext}$. Maps of Doppler boosting factor $\delta$ and observed directions of linear polarization of synchrotron emission are also constructed.

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A. V. Chernoglazov, V. S. Beskin, V. I. Pariev. 2019-12-11. On the Radio Image of Relativistic Jets -- I. Internal Structure, Doppler Boosting, and Polarization Maps. https://doi.org/10.1093/mnras%2Fstz1683

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