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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

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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

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