Water Maser Emission and the Visual Light Curve of R Draconis

Details Water Maser Emission and the Visual Light Curve of R Draconis Water Maser Emission and the Visual Light Curve of R Draconis

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991javso..20..203o&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 20, no. 2, p. 203-207

Physics

R Draconis

Scientific paper

The water maser emmision of R Draconis was observed at 22 GHz at the
Haystack Observatory approximately once each month from November 1988 to
July 1990. There is a correlation between the variations of the maser
emission and the AAVSO light curve; the peak of the maser activity
follows the light activity by about 0.2 period.

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