H2O Observations of Maser Emission of Late Type Variable Stars

Details H2O Observations of Maser Emission of Late Type Variable Stars H2O Observations of Maser Emission of Late Type Variable Stars

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1501....3b&link_type=abstract

Astronomicheskii Tsirkulyar NO.1501/JUL, P. 3, 1987

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Results are presented of monitoring of the 22 GHz H2O maser of the long-period variables U Ori and R Aql. The observations were made with the 22 m Pushchino Radiotelescope in 1983 - 1987. U Ori and R Aql show periodic maser flux variations that are correlated with the visual curve, with a small phase-lag; the H2O maxima are normally delayed by 0.1 to 0.2 cycle with respect to the visual maxima.

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