Microwave Radio Emission from the Red Dwarf Star Yz-Canis

Details Microwave Radio Emission from the Red Dwarf Star Yz-Canis Microwave Radio Emission from the Red Dwarf Star Yz-Canis

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.265..231s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 265, NO. 1/NOV1, P. 231, 1993

Astronomy and Astrophysics

Astronomy

5

Stars: Activity - Stars: Flare - Stars: Individual: Yz Cmi - Radio Continuum: Stars

Scientific paper

We present observations at 5 GHz of flaring and quiescent emission from the red dwarf star YZ CMi, obtained with the Jodrell Bank broad-band interferometer. Weak (1 to 2 mJy) quiescent emission varying over time-scales of hours was detected, in addition to a strong outburst on 1988 October 6 which reached 42 mJy and lasted several minutes. Low-level flaring at ˜15 mJy and of short duration (<20 s) also occurs continuously at a rate of 5 to 6 events per hour.

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