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We have observed eight faint cataclysmic variable stars photometrically. The nova‐like Car2 was extensively sampled but showed little variability. V1040 Cen was observed near the end of a dwarf nova outburst and possessed dwarf nova and quasi‐periodic oscillations. Hα 075648 has strong large amplitude flickering and a possible orbital modulation at 3.49 h. The correct identification for the nova remnant IL Nor (Nova Nor 1893) has been established. HS Pup (Nova Pup 1963) has a possible orbital period of 3.244 h. SDSS  J2048−06  is a low‐mass transfer dwarf nova that in quiescence shows slow variations at 7.67 h (though poorly sampled with our observations) and an orbital modulation at 87.26 min. The dwarf nova CSS  081419−005022  has an orbital period of 1.796 h and the eclipsing dwarf nova CSS  112634−100210  has an orbital period of 1.8581 h.

monthly notices of the royal astronomical society

High speed photometry of faint cataclysmic variables – VI. Car2, V1040 Cen, Hα 075648, IL Nor (Nova Nor 1893), HS Pup (Nova Pup 1963), SDSS  J2048−06 , CSS  081419−005022  and CSS  112634−100210