
%0 Journal Article
%A Tinti, Sara 
%A Dallacasa, Daniele 
%A Stanghellini, Carlo 
%A Celotti, Annalisa 
%T VLBA Observations of Bright High Frequency Peakers
%J Publications of the Astronomical Society of Australia
%D 2003/06/04
%V 20
%N 1
%P 110-112
%K galaxies: active &#8212; quasars: general &#8212; radio continuum: galaxies
%R https://doi.org/10.1071/AS02043
%U https://www.publish.csiro.au/paper/AS02043 
%X The anticorrelation between the turnover frequency in the radio spectrum and the projected linear size (indicative of the age in the currently favoured youth model) in powerful and intrinsically compact radio sources suggests that the youngest objects must have the highest turnover frequencies. We present preliminary results of new VLBA observations of a sample of sources peaking at frequencies higher than a few GHz, making them good candidates for being newly born sources. Our initial analysis deals with the morphological classification which allows us to study the contamination from beamed sources dominated by a single unresolved component. 
