Observations at 843-MHZ of Quiescent Emission from the Flare Star At-Microscopii

Details Observations at 843-MHZ of Quiescent Emission from the Flare Star At-Microscopii Observations at 843-MHZ of Quiescent Emission from the Flare Star At-Microscopii

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.223..399v&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 223, NO.2/NOV15, P. 399, 1986

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Scientific paper

The Molonglo Observatory Synthesis Telescope was used in 1983 and on four occasions in 1985 to map the 843-MHz continuum emission from a field including the flare star AT Mic. Quiescent emission, apparently from the star, was detected. The flux density varied from one observation to another, in the range 3 to 8 mJy at 843 MHz. These observations are thought to be the first reported of quiescent emission from a flare star at such a low frequency. The emission mechanism is not known.

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