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[en] Extensive CCD photometry is presented of the optical counterpart of X1735-444 which reveals the orbital period of the system. It is periodically variable with a period of 4.654 hr and a full amplitude of 0.15 mag. The mean modulation is quasi-sinusoidal; there are, however, also significant intrinsic deviations from the mean light curve. (author)
Journal
Monthly Notices of the Royal Astronomical Society; ISSN 0035-8711; 
; CODEN MNRAA; v. 222(2); p. 15P-19P
; CODEN MNRAA; v. 222(2); p. 15P-19P