RT Ursae Minoris. An eclipsing binary with variable period.

Details RT Ursae Minoris. An eclipsing binary with variable period. RT Ursae Minoris. An eclipsing binary with variable period.

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992geoce..20....1m&link_type=abstract

GEOS Circ., No. EB20, p. 1 - 8

Physics

Scientific paper

All available observations of RT UMi have been analysed. The following ephemeris has been found Min I = 2441306,321 + 1,8419735·E. Relevant O-C values still remain with respect to this ephemeris; this is explained assuming a variable period for the star. The time scale of the variation of O-Cs is around 10000 days, while its amplitude is about 0.04 d. It is not possible to establish the type of period variation.

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