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Water in NGC 1068

Published online by Cambridge University Press:  12 April 2016

L. J. Greenhill
L. J. Greenhill*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, U.S.A.

Abstract

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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.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 221 - 222
Copyright
Copyright © Astronomical Society of the Pacific 1998

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