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Shock Structure of the High-Velocity Water Masers in W 49 N

Published online by Cambridge University Press:  12 April 2016

T. Liljeström
T. Liljeström*
Affiliation:
Metsähovi Radio Research Station, Helsinki University of Technology, Finland

Abstract

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Magnetic field parameters and other characteristics of the postshocked gas in W 49 N are derived from a linewidth comparison between the multi-epoch VLBI data of Gwinn and contemporaneous long-term single-dish observations. The observations support predictions of dissociative shock models.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 251 - 252
Copyright
Copyright © Astronomical Society of the Pacific 1998

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