A search for centimetric wavelength emission from UV Ceti stars

Details A search for centimetric wavelength emission from UV Ceti stars A search for centimetric wavelength emission from UV Ceti stars

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90...93m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, Feb.-Mar. 1978, p. 93-95. Research supported by the Research Corp.

Astronomy and Astrophysics

Astronomy

1

Centimeter Waves, Flare Stars, Radio Astronomy, Radio Emission, Visual Photometry, Light Emission, Radio Frequency Interference

Scientific paper

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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