Abstract
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.
| Original language | English |
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| Pages (from-to) | 399-403 |
| Number of pages | 5 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 223 |
| Issue number | 2 |
| Publication status | Published - 15 Nov 1986 |