Abstract
In 1998, the intensity of the 1.35-cm H2O maser radio line in the source Orion KL increased several hundreds of times. The observations of this flare and its behavior with time are presented.
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Translated from Pis'ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 26, No. 1, 2000, pp. 41–44.
Original Russian Text Copyright © 2000 by Tolmachev.
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Tolmachev, A.M. A flare of the H2O maser in the source Orion KL. Astron. Lett. 26, 34–37 (2000). https://doi.org/10.1134/1.20366
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DOI: https://doi.org/10.1134/1.20366