Proper Motions in Compact Symmetric Objects
By A. Polatidis, J. Conway, I. Owsianik. Publications Astronomical Society of Australia, 2002
137 citations recorded by the source corpus.
Abstract We discuss recent measurements of proper motions of the hotspots of compact symmetric objects (CSOs). Source expansion has been detected in 10 CSOs so far and all these objects are very young (≤ 3 × 103 yr). In a few sources ages have also been estimated from energy supply and spectral ageing arguments and these estimates are comparable. This argues that these sources are close to equipartition and that standard spectral ageing models apply. Proper motion studies are now constraining hotspot accelerations, side-to-side motions, and differences in hotspot advance speeds between the two hotspots of a source. Although most CSOs are young sources their evolution is unclear. There is increasing evidence that in some objects the CSO structure represents a new phase of activity within a recurrent source.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/c6b1c140601a65171e5417f876b0ff126b7acdb5
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
Citations in the corpus
- Radio galaxies and feedback from AGN jets (2020, methodology): “The suggestion that all of these objects (which have nuclear X-ray radiation and VLBI-detected jets in most cases) are simply taking a short break from being radiatively efficient (Tadhunter, 2016) is inconsistent with observations that show other physical differences between LERG and HERG FRIIs at ”