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Combining VLBI and MASIV - how intrinsic properties influence interstellar scintillation of AGN
2012
Proceedings of Resolving The Sky - Radio Interferometry: Past, Present and Future — PoS(RTS2012)
unpublished
Many flat-spectrum AGN exhibit short timescale variations when observed at radio wavelengths, due to interstellar scintillation (ISS). The observed variations depend on source angular size and "core dominance", as well as on the scattering properties of the intervening interstellar medium, both of which are highly non-uniform when considering large samples. ISS offers a powerful probe of source structure on micro-arcsecond angular scales. However, in order to use the statistics of ISS as a
doi:10.22323/1.163.0015
fatcat:2elq47p5kfeiddyzomx27w7s3a