Comparision of Light Variability and Water Maser Emission in T Ursae Majoris

Details Comparision of Light Variability and Water Maser Emission in T Ursae Majoris Comparision of Light Variability and Water Maser Emission in T Ursae Majoris

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988javso..17..120w&link_type=abstract

The Journal of the American Association of Variable Star Observers. vol. 17, no. 1, p. 120-122

Computer Science

3

T Ursae Majoris

Scientific paper

We have observed 22 GHz water maser emission for T UMa at Haystack Observatory about once a month since December 14, 1986. The data have been compiled and graphed as a function of time and compared to the visual data compiled by the AAVSO. The variablilty of the maser emission and the visual light is comparable, but the maser emission shows a phase lag of 0.35 phase with respect to the visible.

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