Variations in the H2O Maser Emission of the source G43.8-0.1 in 1981-1994

Details Variations in the H2O Maser Emission of the source G43.8-0.1 in 1981-1994 Variations in the H2O Maser Emission of the source G43.8-0.1 in 1981-1994

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995azh....72..532l&link_type=abstract

Astronomicheskij Zhurnal, vol. 72, p. 532

Astronomy and Astrophysics

Astronomy

5

Interstellar Masers, Maser Outputs, Star Formation, Line Spectra, Radial Velocity, Emission Spectra, Water Masers, Spatial Distribution

Scientific paper

Results of studies of the total flux variability of the H2O maser source G43.8-0.1, which is associated with a star-forming region, are presented. The observations were made at the 1.35 cm line during 1981-1994 on the RT-22 radio telescope of the Radio Astronomy Station of the Lebedev Institute of Physics in Pushchino. Outburst and long-periodic variability of the maser emission was detected. Six stages of evolution of the maser associated with condensation at a radial velocity of 42.2 km/s are distinguished. A possible origin of the observed phenomena is discussed.

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