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Paper: Shock Structure of the High-Velocity Water Masers in W49 N
Volume: 144, Radio Emission from Galactic and Extragalactic Compact Sources, IAU Colloquium 164
Page: 251
Authors: Liljestroem, T.
Abstract: Magnetic field parameters and other characteristics of the postshocked gas in W49 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.
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