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Masers in Active Galactic Nuclei

Published online by Cambridge University Press:  12 April 2016

L.J. Greenhill*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA

Abstract

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Studies of OH and H2O masers contribute to our understanding of the dynamics and physical conditions in the innermost few parsecs of AGN. Angular and velocity resolutions that may be routinely achieved with radio interferometry are substantially better than those possible with traditional observational techniques in the optical and ultraviolet.

Type
VIII. Megamasers in Active Galaxies
Copyright
Copyright © Astronomical Society of the Pacific 1997

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