Young radio sources: From newly born to short‐lived objects

Abstract

AbstractThe evolutionary stage of a powerful radio source originated by an active galactic nucleus is related to its linear size. Following the evolution models, intrinsically compact objects would evolve into the population of classical radio galaxies. However, the fraction of young radio sources in flux density‐limited samples is much larger than what is expected from the number counts of large radio sources, suggesting the existence of short‐lived objects. We present results of multi‐epoch very large array and very long baseline array observations of a sub‐sample of extreme GPS sources that should be at the very beginning of their radio evolution. We also briefly introduce a new project aiming at determining the incidence of short‐lived objects among a statistically complete sample of young radio sources.