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Evolution of OH and H2O Maser Emission in the Active Star Formation Region NGC 2071
Authors:Ashimbaeva  N T  Colom  P  Krasnov  V V  Lekht  E E  Pashchenko  M I  Rudnitskii  G M  Tolmachev  A M
Institution:1.Moscow State University, Sternberg Astronomical Institute, 119234, Moscow, Russia
;2.Observatoire de Paris-Meudon, Meudon, France
;3.Astro Space Center, Lebedev Physical Institute, 117997, Moscow, Russia
;4.Pushchino Radio Astronomy Observatory, Lebedev Physical Institute, Pushchino, Russia
;
Abstract:Astronomy Reports - We present the observation results of the star forming region NGC 2071 in the 1.35-cm H2O line and 18-cm OH lines obtained with the 22-m radio telescope in Pushchino (Russia)...
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