Abstract
AbstractThe nature and origin of Broad Absorption Line (BAL) quasars and their relationship to non‐BAL quasars are an open question. The BAL quasars are probably normal quasars seen along a particular line of sight. Alternatively, they are young or recently refueled. The high resolution radio morphology of BAL quasars is very important to understand the radio properties of BAL quasars. We present VLBA observations at L and C bands for a sample of BAL quasars. The observations will help us to explore the VLBI radio properties, and distinguish the present models of explaining BAL phenomena. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
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