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We present the results of a photometric campaign of the dwarf nova V1040 Cen.The light curve shows two normal outbursts with recurrence time ~ 40 days andamplitude ~ 2.5 mag. Quiescence data show oscillations with periods in therange ~ 0.1 days (2.4 h) to ~ 0.5 days (12 h) of unknown origin. We measuredthe orbital period of V1040 Cen to be P_orb=0.060458(80) days (1.451+-0.002 h).Based on the M_v-P_orb relation we found the distance of V1040 Cen to be137+-31 pc. In this paper we also report the detection of eleven new variablestars in the field of the monitored dwarf nova.

Dwarf Nova V1040 Centauri and Variable Stars in its Vicinity