Hostname: page-component-77c89778f8-9q27g Total loading time: 0 Render date: 2024-07-18T06:41:28.617Z Has data issue: false hasContentIssue false
  • English
  • Français

Global Oscillations of Masing Disks in Megamasers

Published online by Cambridge University Press:  25 May 2016

Atsuo T. Okazaki
Atsuo T. Okazaki*
Affiliation:
Faculty of Engineering, Hokkai-Gakuen University, Toyohira-ku, Sapporo 062-8605, Japan

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 study the characteristics of global oscillation modes of masing disks in megamasers and the effect of the modes on the disk kinematics. We find that the eccentric mode is responsible for the observed sub-Keplerian velocity distribution of the maser source of NGC 1068, whereas in the masing disk of NGC 4258 the warping mode is dominant so that the angular rotation velocity remains near Keplerian.

Type
I. Observational Properties of AGN
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 90 - 91
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Miyoshi, M., Moran, J., Herrnstein, J., Greenhill, L., Nakai, N., Diamond, P., and Inoue, M. 1995, Nat, 373, 127 CrossRefGoogle Scholar
Greenhill, L. J., Gwinn, C. R., Antonucci, R., and Barvainis, R. 1996, Ap.J., 472, L21 CrossRefGoogle Scholar