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.
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CITATION STYLE
APA
Bignall, H., Macquart, J.-P., Godfrey, L., Hodgson, J., & Jauncey, D. (2014). Microarcsecond structure of an AGN Jet via Interstellar Scintillation. Proceedings of the International Astronomical Union, 10(S313), 143–144. https://doi.org/10.1017/s1743921315002082
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