A radio survey of cataclysmic variable stars using the very large array

Details A radio survey of cataclysmic variable stars using the very large array A radio survey of cataclysmic variable stars using the very large array

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pasp...95...69c&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 95, Jan. 1983, p. 69-71. Research supported by the U.S. Department of En

Astronomy and Astrophysics

Astronomy

14

Binary Stars, Radio Astronomy, Stellar Magnetic Fields, Stellar Mass Accretion, Variable Stars, Very Large Array (Vla), Dwarf Stars, Magnetic Stars, Thermal Emission

Scientific paper

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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