A method of using AGNs as cosmological probes and some recent results
are discussed. The method is based on fitting the Hedgehog model to ob
servations of spectra, structure and polarization of AGN radio emissio
n and time variations of the observed quantities. If red shifts of sel
ected AGNs are known, extragalactic distances, the Hubble constant and
the deceleration parameter of the Universe can be measured using only
radio observations. Recent results may give new strong arguments for
the basic model to be in agreement with observations of variable spect
ra and structure of many AGNs, and may allow preliminary selection of
AGNs for further use.