2002PASP..114..623K

We present photometry and spectroscopy of HT Camelopardalis, a recently discovered X-ray-bright cataclysmic variable. The spectrum shows bright lines of H, He I, and He II, all moving with a period of 0.059712(1) days, which we interpret as the orbital period. The star's brightness varies with a strict period of 515.0592(2) s and a mean full amplitude of 0.11 mag. These properties qualify it as a bona fide DQ Herculis star (intermediate polar), in which the magnetism of the rapidly rotating white dwarf channels accretion flow to the surface. Normally at V=17.8, the star shows rare and very brief outbursts to V=12-13. We observed one in 2001 December and found that the 515 s pulse amplitude had increased by a factor of ∼100 (in flux units). A transient orbital signal may have appeared as well.