Improved Orbital Ephemeris of GT Ursae Majoris

Details Improved Orbital Ephemeris of GT Ursae Majoris Improved Orbital Ephemeris of GT Ursae Majoris

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ibvs.5530....1m&link_type=abstract

Information Bulletin on Variable Stars, 5530, 1.

Physics

Period Variation, O-C Study

Scientific paper

Extensive B and V CCD photometry of GT UMa is reported. It is used to
derive an improved orbital ephemeris and observe that GT UMa is a
detached system of two F2 stars of equal temperature.

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