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A search for centimetric wavelength emission from UV Ceti stars
Journal article

A search for centimetric wavelength emission from UV Ceti stars

T. J Moffett, H. F Helmken and S. R Spangler
Publications of the Astronomical Society of the Pacific, Vol.90(533), pp.93-95
02/1978
DOI: 10.1086/130284

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Abstract

Simultaneous radio and optical observations were obtained on three UV Cet flare stars: YZ CMi, AD Leo, and Wolf 424. The total simultaneous monitoring time was 33.9 hours during which time 41 optical flares were detected. Two enhancements were detected at 1420 MHz in close temporal association with optical flares, but are of uncertain validity. The results presented indicate that 1420 MHz emission during a typical stellar flare is less than 0.10 Jy

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