Radio emission of cataclysmic variable stars

Details Radio emission of cataclysmic variable stars Radio emission of cataclysmic variable stars

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...154..377f&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 154, no. 1-2, Jan. 1986, p. 377, 378. Research supported by the Swiss Society

Astronomy and Astrophysics

Astrophysics

7

Cataclysmic Variables, Radio Emission, Stellar Radiation, Bremsstrahlung, Magnetic Fields, Optical Thickness, Relativistic Electron Beams, Very Large Array (Vla)

Scientific paper

Eight cataclysmic variable stars were observed at 6 cm wavelength using
the Very Large Array (VLA). The objects were: CN Ori, SS Aur, YZ Cnc, SU
UMa, Z Cam, V603 Aql, EM Cyg, and RZ Sge. Most of these objects were in
optical high stage, but none were detected beyond flux limits between
0.1 and 0.3 mJy.

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