High-resolution radio observations of the Seyfert galaxy NGC 1068

Abstract
High-resolution (≲ 1 arcsec) MERLIN observations at 73 and 18 cm of the nucleus of NGC 1068 are presented. The 18-cm radio structure strongly suggests the presence of a radio jet emanating from a central component. This central component is smaller than 1 arcsec and shows a low-frequency turnover which is interpreted as being due to free–free absorption by clouds in the forbidden-line region (FLR). It is estimated that a typical FLR cloud has a mass of ∼ 1 M and from this it is argued that the beam velocity of the jet could be of order 103 Km s−1.

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