No CrossRef data available.
Article contents
Relativistic Electron-Positron Clouds in VLBI Jets
Published online by Cambridge University Press: 25 May 2016
Extract
Extragalactic jets have always had two characteristics : the presence of knots and the requirement for particle acceleration. Shock fronts provide an explanation for both. However, the knotty appearance is less obvious at kp-scale on very high resolution observations from the VLA and the HST. The evidence for shock fronts is therefore weakened. At the pc-scale (or VLBI scale), a lot of these blobs are moving superluminally and they have been interpreted and modelled as shock fronts in a relativistic jet.
- Type
- Radio Source Modelling and Emission Mechanisms
- Information
- Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 443 - 444
- Copyright
- Copyright © Kluwer 1996