Hostname: page-component-788cddb947-w95db Total loading time: 0 Render date: 2024-10-14T07:50:23.302Z Has data issue: false hasContentIssue false
  • English
  • Français

The H2O Supermaser Emission Region in Orion KL

Published online by Cambridge University Press:  12 April 2016

L. I. Matveenko ,
P. J. Diamond  and
D. A. Graham
L. I. Matveenko
Affiliation:
Space Research Institute, Moscow 117810, Russia
P. J. Diamond
Affiliation:
National Radio Astronomy Observatory, Socorro, NM, U.S.A.
D. A. Graham
Affiliation:
Max-Planck-Institut für Radioastronomie, 53121 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 compare spatial structure of the H20 maser during an active period with that during a later quiescent period, received with VLBA in 1993.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 249 - 250
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Abraham, Z., et al. 1981. A&A, 100, L10–13.Google Scholar
Garay, G., Moran, J.M., & Hashick, A.D. 1989, ApJ, 338, 244–261.Google Scholar
Matveenko, L.I. 1981. Soviet Ast. Lett., 7, 54–57.Google Scholar
Matveenko, L.I., Graham, D.A., & Diamond, P.J. 1988. Soviet Ast. Lett., 14, 468–476.Google Scholar
Matveenko, L.I., & Diamond, P.J. 1994. in VLBI Technology, Progress, and Future Observational Possibilities, eds. Sasao, T., Manabe, S., Kameya, O., & Inoue, M. (Tokyo: Terra), 105–109.Google Scholar