Microarcsecond structure of an AGN Jet via Interstellar Scintillation
arXiv:1502.03739 · doi:10.1017/S1743921315002082
Abstract
We have used the broadband backend available at the ATCA to study the fast interstellar scintillation 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.
2 pages, 1 figure, to appear in Proceedings of IAU Symposium 313: Extragalactic Jets from every angle