Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-27T04:33:13.436Z Has data issue: false hasContentIssue false
  • English
  • Français

Shock Origin of High-Velocity Maser Emission from Circumnuclear Disks

Published online by Cambridge University Press:  12 April 2016

Eyal Maoz  and
Christopher F. McKee
Eyal Maoz
Affiliation:
Astronomy Department, University of California at Berkeley Miller Fellow
Christopher F. McKee
Affiliation:
Astronomy Department, University of California at Berkeley Physics Department, University of California at Berkeley

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 propose that the observed high-velocity maser emission from circumnuclear disks arises in spiral shocks, which can naturally account for several peculiar findings in the spectrum and spatial distribution of the maser emission.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 217 - 218
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Greenhill, L.J., et al. 1996. ApJ, 472, L21–24.CrossRefGoogle Scholar
Greenhill, L.J., Moran, J.M., & Herrnstein, J.R. 1997. ApJ, 481, L23–26.CrossRefGoogle Scholar
Maoz, E., & McKee, C.F. 1997. ApJ, in press.Google Scholar
Miyoshi, M., et al. 1995. Nature, 373, 127–129.Google Scholar