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NGC 1052: A Different Class of H2O Megamaser?

Published online by Cambridge University Press:  12 April 2016

P. J. Diamond ,
M. J. Claussen ,
J. A. Braatz ,
A. S. Wilson  and
C. Henkel
P. J. Diamond
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
M. J. Claussen
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
J. A. Braatz
Affiliation:
Center for Astrophysics, Cambridge, MA 02138, U.S.A.
A. S. Wilson
Affiliation:
University of Maryland, Astronomy Dept., College Park, MD 20742, U.S.A.
C. Henkel
Affiliation:
Max-Planck-Institut f. Radioastronomie, 53010 Bonn, Germany

Abstract

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We present VLBA observations of the H2O megamasers in the LINER galaxy NGC 1052. The structure we observe suggests a different origin for the masers than those seen in NGC 4258.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 223 - 224
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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