Data di Pubblicazione:
2003
Abstract:
On the basis of the different radio properties (especially different radio
morphologies) between GPS galaxies and GPS quasars, I suggest that GPS
galaxies are a more homogeneous class mainly consisting of compact symmetric
objects, while the majority of GPS quasars are an intrinsically different
type of radio source, similar to the common flat spectrum radio sources.
For CSS radio sources the difference between galaxies and quasars is less
evident. This is interpreted as a bias correlated with size: samples of
smaller objects are more likely to be contaminated by unrelated objects.
This is consistent also with the high percentage of blazar/quasar objects
present in a sample of the even smaller HFP radio sources.
Tipologia CRIS:
01.01 Articolo in rivista
Elenco autori:
Stanghellini, Carlo
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