Abstract
It is argued that the unresolved VLBI-cores in flat spectrum, compact radio sources have properties very similar to the associated blazar emission region: Large scale magnetic field, anisotropic pitch-angle distribution and the importance of relativistic streaming motion. Problems afflicting models invoking Compton-cooling behind a relativistic shock in a jet to explain the initial phase of out-bursts in the mm/far-infrared regime are discussed. As an alternative, a qualitative discussion is given of a model where relativistic streaming and pitch-angle scattering are the main ingredients.
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© 1991 Springer-Verlag
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Björnsson, CI. (1991). The connection between blazars and compact radio sources. In: Duschl, W.J., Wagner, S.J., Camenzind, M. (eds) Variability of Active Galaxies. Lecture Notes in Physics, vol 377. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0030059
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DOI: https://doi.org/10.1007/BFb0030059
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