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Water in NGC 1068

Published online by Cambridge University Press:  12 April 2016

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
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Brinks, E., et al. 1997. Ap&SS, 248, 2331.Google Scholar
Gallimene, J.F., Baum, S.A., O’Dea, C.P. 1997. Nature, 388, 852854.CrossRefGoogle Scholar
Gallimore, J.F., et al. 1996. ApJ, 462, 740745.CrossRefGoogle Scholar
Greenhill, L.J., et al. 1996. ApJ, 472, L2124.CrossRefGoogle Scholar
Gwinn, C.R., et al. 1993. In Sub-Arcsecond Radio Astronomy, eds. Davis, R.J. & Booth, R.S. (Cambridge: Cambridge University Press), 331332.Google Scholar
Helfer, T.T., & Blitz, L. 1995. ApJ, 450, 90110.CrossRefGoogle Scholar
Herrnstein, J.R., et al. 1997. ApJ, 475, L1721.CrossRefGoogle Scholar
Miyoshi, M., et al. 1995. Nature, 373, 127130.CrossRefGoogle Scholar
Pier, E.A., et al. 1994. ApJ, 428, 124129.CrossRefGoogle Scholar
Tacconi, L.J., et al. 1994. ApJ, 426, L7780.CrossRefGoogle Scholar