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Water Maser Emission and the Parsec–Scale Jet in NGC 3079

Published online by Cambridge University Press:  12 April 2016

A. S. Trotter ,
J. M. Moran  and
L. J. Greenhill
A. S. Trotter
Affiliation:
Harvard-Smithsonian CfA, Cambridge, MA 02138, U.S.A.
J. M. Moran
Affiliation:
Harvard-Smithsonian CfA, Cambridge, MA 02138, U.S.A.
L. J. Greenhill
Affiliation:
Harvard-Smithsonian CfA, Cambridge, MA 02138, U.S.A.

Abstract

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We have imaged the H2O maser and 22, 8, & 5 GHz continuum in the nucleus of NGC 3079, using the NRAO VLBA. The maser features are distributed over ~ 2 pc along an axis aligned with the plane of the kpc–scale edge–on molecular disk. The masers are not angularly coincident with any detected continuum emission. The two brightest continuum features, which trace a parsec–scale jet, have similar spectra that peak at frequencies ν > 5 GHz. We also detected faint maser emission along the jet axis.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 239 - 240
Copyright
Copyright © Astronomical Society of the Pacific 1998

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