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Water in NGC 1068
Published online by Cambridge University Press: 12 April 2016
Abstract
We report the first VLBI images of the NGC 1068 H2O maser that include the full 600 km s−1 spread of the emission. The structure of the source is suggestive of an edge-on massive disk that is probably bound by the central engine of this AGN.
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- Copyright © Astronomical Society of the Pacific 1998
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