Compact Symmetric Objects (CSOs) are considered the young counterparts of large doubles according to advance speeds measured or inferred from spectral ageing. Here we present a simple power law model for the CSO/FRII evolution based on the study of sources with well defined hot-spots. The luminosity of the hot spots is estimated under minimum energy conditions. The advance of the source is considered to proceed in ram pressure equilibrium with the ambient medium. Finally, we also assume that the jets feeding the hot spots are relativistic and have a time dependent power. Comparison with observational data allows to interpret the CSO-FRII evolution in terms of decreasing jet power with time
We constrain the spectral ages for two very asymmetric Compact Symmetric Objects (CSO) from the B3-V...
Context. The compact symmetric objects (CSOs) are small (< 1 kiloparsec) and powerful extragalactic ...
There is mounting evidence that mechanical radio source feedback is important in galaxy evolution an...
Compact symmetric objects conform a class of sources characterized by high luminosity radio emission...
The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth ...
The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth ...
We discuss recent measurements of proper motions of the hotspots of Compact Symmetric Objects. Sourc...
Double lobe radio sources associated with active galactic nuclei represent one of the longest studie...
Aims.We constrain the spectral ages for two very asymmetric Compact Symmetric Objects (CSO) from the...
We present an analytical model for the cosmological evolution of the FR II source population. Based ...
This is the second in a series of papers presenting an analytical model for the evolu-tion of FRII r...
The measurement of proper motions in CSOs is a powerful tool to determine the dynamical evolution of...
Open AccessFor a representative sample of 10 bright hot spots associated with classical double radio...
Observations of 10 Compact Symmetric Object (CSO) candidates have been made with the Very Long Basel...
This is the second in a series of papers presenting an analytical model for the evolution of Fanarof...
We constrain the spectral ages for two very asymmetric Compact Symmetric Objects (CSO) from the B3-V...
Context. The compact symmetric objects (CSOs) are small (< 1 kiloparsec) and powerful extragalactic ...
There is mounting evidence that mechanical radio source feedback is important in galaxy evolution an...
Compact symmetric objects conform a class of sources characterized by high luminosity radio emission...
The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth ...
The evolution of symmetric extragalactic radio sources can be characterized by four distinct growth ...
We discuss recent measurements of proper motions of the hotspots of Compact Symmetric Objects. Sourc...
Double lobe radio sources associated with active galactic nuclei represent one of the longest studie...
Aims.We constrain the spectral ages for two very asymmetric Compact Symmetric Objects (CSO) from the...
We present an analytical model for the cosmological evolution of the FR II source population. Based ...
This is the second in a series of papers presenting an analytical model for the evolu-tion of FRII r...
The measurement of proper motions in CSOs is a powerful tool to determine the dynamical evolution of...
Open AccessFor a representative sample of 10 bright hot spots associated with classical double radio...
Observations of 10 Compact Symmetric Object (CSO) candidates have been made with the Very Long Basel...
This is the second in a series of papers presenting an analytical model for the evolution of Fanarof...
We constrain the spectral ages for two very asymmetric Compact Symmetric Objects (CSO) from the B3-V...
Context. The compact symmetric objects (CSOs) are small (< 1 kiloparsec) and powerful extragalactic ...
There is mounting evidence that mechanical radio source feedback is important in galaxy evolution an...