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CCD photometry of the classical nova RW UMi during 10 nights in 1995 throughan R filter and 14 nights in 1997 through a `clear' filter, with the 1-m Wisetelescope yields a periodic modulation in the light curve with the period0.05912+/-0.00015 d and a semi amplitude of 0.025 mag. We discuss severalexplanations for the periodicity, and suggest that it is likely to be theorbital period of the binary system or a superhump period. RW UMi is thus acandidate for the classical nova with the shortest known orbital period.Comment: 6 pages, 3 eps. figures, Latex, A&A in pres

The detection of a 1.4-h period in RW Ursa Minoris -candidate for shortest recorded orbital period nova