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Structure and Properties of AGN Cores from VLBI and Total Flux Density Variations
Published online by Cambridge University Press: 12 April 2016
Abstract
By combining VLBI and total flux density data it is possible to get an indirect “look” at the innermost, unresolved core regions of AGN and to estimate physical parameters such as the intrinsic brightness temperatures, Lorentz factors and viewing angles, unobtainable by either VLBI or multi-frequency flux monitoring alone.
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- Copyright © Astronomical Society of the Pacific 1998