Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-27T04:47:06.119Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Braatz, J.A., et al. 1994. ApJ, 437, L99–103.Google Scholar
Gallimore, J.F., et al. 1996. ApJ, 464, 198–211.Google Scholar
Greenhill, L.J., et al. 1996. ApJ, 472, L21–25.Google Scholar
Koekemoer, A.M., et al. 1995. Nature, 378, 679–671.CrossRefGoogle Scholar
Miyoshi, M., et al. 1995. Nature, 373, 127–129.CrossRefGoogle Scholar