1983/01/01 by F. A. Cordova, F. A. Córdova, R. M. Hjellming +1
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #History and Developments in Astronomy #Astrophysical Phenomena and Observations
paper · pdf · doi:10.1086/131119
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.