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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
Abstract
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.
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- Copyright © Astronomical Society of the Pacific 1998