Models of the brightness temperature distributions in compact, extragalactic radio jets

Astronomy and Astrophysics – Astronomy

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Scientific paper

The brightness temperature distribution is a powerful tool to study the conditions in the extragalactic radio sources and to test the models proposed for the inner jets. In this talk we will present the model which describes the brightness temperature distribution in terms of randomly oriented source and a) a single value for the intrinsic brightness temperature and Lorentz factor or b) a function which describes the distribution of these two parameters.

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