ST Ursae Majoris: An Interesting Binocular Variable Star

Details ST Ursae Majoris: An Interesting Binocular Variable Star ST Ursae Majoris: An Interesting Binocular Variable Star

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986javso..15..278s&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 15, no. 2, p. 278

Physics

Scientific paper

Observations of the semiregular star, ST Ursae Majoris, show an
approximate period of 81 days. However, there are occasions when the
period is as long as approximately 120 days or as short as approximately
60 days. In 1980 - 81, one cycle lasted approximately 150 days.

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