Abstract

ABSTRACTPhotometric and spectroscopic observations of the candidate cataclysmic variable KUV 03580+0614, independently found from the Hamburg Survey as HS 0357+0614, reveal this to be a cataclysmic variable with an orbital period of 3.4 hr. Cataclysmic variables with periods in this range are usually nova‐like variables belonging to the SW Sex or intermediate polar categories. The variability, spectroscopic characteristics, and the lack of strong X‐rays indicate a system similar to V795 Her, LS Peg, and AH Men.

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