Abstract
ABSTRACT Six cataclysmic variable stars were searched for 6-cm emission using the NRAO Very Large Array. The candidate stars were SS Cyg, U Gem, TT Ari, RW Sex, EX Hya, and A0 Psc (H2252-035). None were detected; the flux density range between 0.1 and 0.4 mJy. These limits are, respectively, between a factor of 6 and 1.5 lower than the 6-cm emission detected from the magnetic binary AM Her by Chanmugam and Dulk.
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