CCD photometry of the dwarf nova ASASSN-18iq revealing superhumps
To clarify physical processes in dwarf novae accretion disks it is sufficient to operate a telescope with a mirror less than one meter in diameter and to use several observational hours. According to our observations with Zeiss 60-cm telescope, the dwarf nova ASASSN-18iq of SU Ursae Majoris type during a superoutburst of 2018 showed positive superhumps with a mean period of 0.05982 days.