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Observations of variability of H2O Maser sources associated with star formation regions
Published online by Cambridge University Press: 03 August 2017
Abstract
An outstanding feature of the water maser emission from star formation regions is the strong time variability, which was recognised soon after the discovery of interstellar H2O masers. It is likely that the observed considerable variations of the H2O line profiles as well as of the flux density reflect the disturbancies in the protostellar nebule probably associated with the outflow from the newly formed stars.
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