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Microarcsecond structure of an AGN Jet via Interstellar Scintillation
Published online by Cambridge University Press: 24 March 2015
Abstract
We have used the broadband backend available at the ATCA to study the fast interstellar scintillation (ISS) of quasar PKS 1257–326, resolving the core shift as a function of frequency on scales less than 10 microarcseconds. In this short paper we discuss the jet direction implied from the microarcsecond-scale core shift in PKS 1257–326.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 10 , Issue S313: Extragalactic jets from every angle , September 2014 , pp. 143 - 144
- Copyright
- Copyright © International Astronomical Union 2015